{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1360294643775306752.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.3847/1538-4365/ac1432"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4365/ac1432"}},{"identifier":{"@type":"URI","@value":"https://iopscience.iop.org/article/10.3847/1538-4365/ac1432/pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.2109.06268"}},{"identifier":{"@type":"HANDLE","@value":"1887/3275450"}},{"identifier":{"@type":"HANDLE","@value":"10023/28597"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). I. Program Overview and Highlights"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>Planets form and obtain their compositions in dust- and gas-rich disks around young stars, and the outcome of this process is intimately linked to the disk chemical properties. The distributions of molecules across disks regulate the elemental compositions of planets, including C/N/O/S ratios and metallicity (O/H and C/H), as well as access to water and prebiotically relevant organics. Emission from molecules also encodes information on disk ionization levels, temperature structures, kinematics, and gas surface densities, which are all key ingredients of disk evolution and planet formation models. The Molecules with ALMA at Planet-forming Scales (MAPS) ALMA Large Program was designed to expand our understanding of the chemistry of planet formation by exploring disk chemical structures down to 10 au scales. The MAPS program focuses on five disks—around IM Lup, GM Aur, AS 209, HD 163296, and MWC 480—in which dust substructures are detected and planet formation appears to be ongoing. We observed these disks in four spectral setups, which together cover ∼50 lines from over 20 different species. This paper introduces the Astrophysical Journal Supplement’s MAPS Special Issue by presenting an overview of the program motivation, disk sample, observational details, and calibration strategy. We also highlight key results, including discoveries of links between dust, gas, and chemical substructures, large reservoirs of nitriles and other organics in the inner disk regions, and elevated C/O ratios across most disks. We discuss how this collection of results is reshaping our view of the chemistry of planet formation.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380294643775306888","@type":"Researcher","foaf:name":[{"@value":"Karin I. Öberg"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307136","@type":"Researcher","foaf:name":[{"@value":"Viviana V. Guzmán"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307682","@type":"Researcher","foaf:name":[{"@value":"Catherine Walsh"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306781","@type":"Researcher","foaf:name":[{"@value":"Yuri Aikawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307009","@type":"Researcher","foaf:name":[{"@value":"Edwin A. Bergin"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307533","@type":"Researcher","foaf:name":[{"@value":"Charles J. Law"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306909","@type":"Researcher","foaf:name":[{"@value":"Ryan A. Loomis"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307546","@type":"Researcher","foaf:name":[{"@value":"Felipe Alarcón"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307658","@type":"Researcher","foaf:name":[{"@value":"Sean M. Andrews"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307158","@type":"Researcher","foaf:name":[{"@value":"Jaehan Bae"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307290","@type":"Researcher","foaf:name":[{"@value":"Jennifer B. Bergner"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306881","@type":"Researcher","foaf:name":[{"@value":"Yann Boehler"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307013","@type":"Researcher","foaf:name":[{"@value":"Alice S. Booth"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307292","@type":"Researcher","foaf:name":[{"@value":"Arthur D. Bosman"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307401","@type":"Researcher","foaf:name":[{"@value":"Jenny K. Calahan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306762","@type":"Researcher","foaf:name":[{"@value":"Gianni Cataldi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306628","@type":"Researcher","foaf:name":[{"@value":"L. Ilsedore Cleeves"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307282","@type":"Researcher","foaf:name":[{"@value":"Ian Czekala"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307402","@type":"Researcher","foaf:name":[{"@value":"Kenji Furuya"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306892","@type":"Researcher","foaf:name":[{"@value":"Jane Huang"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306784","@type":"Researcher","foaf:name":[{"@value":"John D. Ilee"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307525","@type":"Researcher","foaf:name":[{"@value":"Nicolas T. Kurtovic"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306880","@type":"Researcher","foaf:name":[{"@value":"Romane Le Gal"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307151","@type":"Researcher","foaf:name":[{"@value":"Yao Liu"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307138","@type":"Researcher","foaf:name":[{"@value":"Feng Long"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307543","@type":"Researcher","foaf:name":[{"@value":"François Ménard"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306635","@type":"Researcher","foaf:name":[{"@value":"Hideko Nomura"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306914","@type":"Researcher","foaf:name":[{"@value":"Laura M. Pérez"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307276","@type":"Researcher","foaf:name":[{"@value":"Chunhua Qi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307269","@type":"Researcher","foaf:name":[{"@value":"Kamber R. Schwarz"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307548","@type":"Researcher","foaf:name":[{"@value":"Anibal Sierra"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307691","@type":"Researcher","foaf:name":[{"@value":"Richard Teague"}]},{"@id":"https://cir.nii.ac.jp/crid/1420845751137575424","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"20533566"},{"@type":"NRID","@value":"1000020533566"},{"@type":"NRID","@value":"9000406062964"},{"@type":"NRID","@value":"9000018861236"},{"@type":"NRID","@value":"9000244901623"},{"@type":"NRID","@value":"9000014145958"},{"@type":"NRID","@value":"9000340952927"},{"@type":"NRID","@value":"9000356566699"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/ttsuka"}],"foaf:name":[{"@value":"Takashi Tsukagoshi"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306898","@type":"Researcher","foaf:name":[{"@value":"Yoshihide Yamato"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307139","@type":"Researcher","foaf:name":[{"@value":"Merel L. R. van ’t Hoff"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307684","@type":"Researcher","foaf:name":[{"@value":"Abygail R. Waggoner"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775307532","@type":"Researcher","foaf:name":[{"@value":"David J. Wilner"}]},{"@id":"https://cir.nii.ac.jp/crid/1380294643775306884","@type":"Researcher","foaf:name":[{"@value":"Ke Zhang"}]}],"contributor":[{"@id":"https://cir.nii.ac.jp/crid/1891992115493923459","@type":"Researcher","foaf:name":[{"@value":"Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) ; Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (Fédération OSUG)-Université Grenoble Alpes (UGA)"}]},{"@id":"https://cir.nii.ac.jp/crid/1891992115493923457","@type":"Researcher","foaf:name":[{"@value":"University of St Andrews.School of Physics and Astronomy"}]},{"@id":"https://cir.nii.ac.jp/crid/1891992115493923460","@type":"Researcher","foaf:name":[{"@value":"Institut de Planétologie et d'Astrophysique de Grenoble (IPAG)"}]},{"@id":"https://cir.nii.ac.jp/crid/1894242817205443603","@type":"Researcher","foaf:name":[{"@value":"ANR-16-CE31-0013,PLANET-FORMING-DISKS,De meilleurs modèles pour de meilleures données(2016)"}]},{"@id":"https://cir.nii.ac.jp/crid/1894242817205443600","@type":"Researcher","foaf:name":[{"@value":"Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) ; Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ) ; Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France"}]},{"@id":"https://cir.nii.ac.jp/crid/1891992115493923456","@type":"Researcher","foaf:name":[{"@value":"Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France"}]},{"@id":"https://cir.nii.ac.jp/crid/1894242817205443602","@type":"Researcher","foaf:name":[{"@value":"Institut de Planétologie et d'Astrophysique de Grenoble (IPAG) ; Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ) ; Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Météo-France"}]},{"@id":"https://cir.nii.ac.jp/crid/1894242817205443623","@type":"Researcher","foaf:name":[{"@value":"University of St Andrews. School of Physics and Astronomy"}]},{"@id":"https://cir.nii.ac.jp/crid/1891992115493923458","@type":"Researcher","foaf:name":[{"@value":"Centre National d'Études Spatiales Toulouse (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG )"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00670049"},{"@type":"EISSN","@value":"15384365"}],"prism:publicationName":[{"@value":"The Astrophysical Journal Supplement Series"}],"dc:publisher":[{"@value":"American Astronomical Society"}],"prism:publicationDate":"2021-11-01","prism:volume":"257","prism:number":"1","prism:startingPage":"1"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["https://iopscience.iop.org/page/copyright","https://iopscience.iop.org/info/page/text-and-data-mining"],"url":[{"@id":"https://iopscience.iop.org/article/10.3847/1538-4365/ac1432"},{"@id":"https://iopscience.iop.org/article/10.3847/1538-4365/ac1432/pdf"}],"createdAt":"2021-11-03","modifiedAt":"2024-01-17","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20instrumentation%20and%20methods%20for%20astrophysics","dc:title":"Astrophysics - instrumentation and methods for astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Protoplanetary%20disks","dc:title":"Protoplanetary disks"},{"@id":"https://cir.nii.ac.jp/all?q=1300","dc:title":"1300"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20astrophysics%20of%20galaxies","dc:title":"Astrophysics - astrophysics of galaxies"},{"@id":"https://cir.nii.ac.jp/all?q=Protoplanetary%20disks%20(1300)","dc:title":"Protoplanetary disks (1300)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=Submillimeter%20astronomy%20(1647)","dc:title":"Submillimeter astronomy (1647)"},{"@id":"https://cir.nii.ac.jp/all?q=1061","dc:title":"1061"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Earth%20and%20planetary%20astrophysics","dc:title":"Astrophysics - Earth and planetary astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Planet%20formation%20(1241)","dc:title":"Planet formation (1241)"},{"@id":"https://cir.nii.ac.jp/all?q=Astrobiology%20(74)","dc:title":"Astrobiology (74)"},{"@id":"https://cir.nii.ac.jp/all?q=Millimeter%20astronomy","dc:title":"Millimeter astronomy"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20solar%20and%20stellar%20astrophysics","dc:title":"Astrophysics - solar and stellar astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=1241","dc:title":"1241"},{"@id":"https://cir.nii.ac.jp/all?q=Millimeter%20astronomy%20(1061)","dc:title":"Millimeter astronomy (1061)"},{"@id":"https://cir.nii.ac.jp/all?q=QB%20Astronomy","dc:title":"QB Astronomy"},{"@id":"https://cir.nii.ac.jp/all?q=1647","dc:title":"1647"},{"@id":"https://cir.nii.ac.jp/all?q=Instrumentation%20and%20Methods%20for%20Astrophysics%20(astro-ph.IM)","dc:title":"Instrumentation and Methods for Astrophysics (astro-ph.IM)"},{"@id":"https://cir.nii.ac.jp/all?q=QC","dc:title":"QC"},{"@id":"https://cir.nii.ac.jp/all?q=Solar%20and%20Stellar%20Astrophysics%20(astro-ph.SR)","dc:title":"Solar and Stellar Astrophysics (astro-ph.SR)"},{"@id":"https://cir.nii.ac.jp/all?q=QB","dc:title":"QB"},{"@id":"https://cir.nii.ac.jp/all?q=Astrochemistry","dc:title":"Astrochemistry"},{"@id":"https://cir.nii.ac.jp/all?q=Planet%20formation","dc:title":"Planet formation"},{"@id":"https://cir.nii.ac.jp/all?q=Earth%20and%20Planetary%20Astrophysics%20(astro-ph.EP)","dc:title":"Earth and Planetary Astrophysics (astro-ph.EP)"},{"@id":"https://cir.nii.ac.jp/all?q=75,%201300,%201241,%2074,%201061,%201647","dc:title":"75, 1300, 1241, 74, 1061, 1647"},{"@id":"https://cir.nii.ac.jp/all?q=75","dc:title":"75"},{"@id":"https://cir.nii.ac.jp/all?q=74","dc:title":"74"},{"@id":"https://cir.nii.ac.jp/all?q=DAS","dc:title":"DAS"},{"@id":"https://cir.nii.ac.jp/all?q=Astrobiology","dc:title":"Astrobiology"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Astrophysics%20of%20Galaxies","dc:title":"Astrophysics - Astrophysics of Galaxies"},{"@id":"https://cir.nii.ac.jp/all?q=520","dc:title":"520"},{"@id":"https://cir.nii.ac.jp/all?q=QC%20Physics","dc:title":"QC Physics"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Solar%20and%20Stellar%20Astrophysics","dc:title":"Astrophysics - Solar and Stellar Astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=%5BSDU%5DSciences%20of%20the%20Universe%20%5Bphysics%5D","dc:title":"[SDU]Sciences of the Universe [physics]"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20of%20Galaxies%20(astro-ph.GA)","dc:title":"Astrophysics of Galaxies (astro-ph.GA)"},{"@id":"https://cir.nii.ac.jp/all?q=Astrochemistry%20(75)","dc:title":"Astrochemistry (75)"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Instrumentation%20and%20Methods%20for%20Astrophysics","dc:title":"Astrophysics - Instrumentation and Methods for Astrophysics"},{"@id":"https://cir.nii.ac.jp/all?q=Submillimeter%20astronomy","dc:title":"Submillimeter astronomy"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Earth%20and%20Planetary%20Astrophysics","dc:title":"Astrophysics - Earth and Planetary Astrophysics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781994779520","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18H05222"},{"@type":"JGN","@value":"JP18H05222"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18H05222/"}],"notation":[{"@language":"ja","@value":"原始惑星系円盤形成領域の化学組成とその進化"},{"@language":"en","@value":"Chemical Composition of Disk Forming Regions of Solar-type Protostars and its Evolution to Planetary Systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781994907392","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18H05441"},{"@type":"JGN","@value":"JP18H05441"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-18H05441/"}],"notation":[{"@language":"ja","@value":"多様な環境下における原始惑星系円盤進化の観測的解明"},{"@language":"en","@value":"Observational Studies on the Evolution of Protoplanetary Disks in Diverse Environments"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782017269888","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19K03910"},{"@type":"JGN","@value":"JP19K03910"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19K03910/"}],"notation":[{"@language":"ja","@value":"原始惑星系円盤から太陽系へ：有機分子の化学進化"},{"@language":"en","@value":"From Protoplanetary Disks to the Solar System: Chemical Evolution of Organic Molecules"}]},{"@id":"https://cir.nii.ac.jp/crid/1040850857186466432","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"21K13967"},{"@type":"JGN","@value":"JP21K13967"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-21K13967/"}],"notation":[{"@language":"ja","@value":"ダストの合体成長に伴う原始惑星系円盤の化学構造進化"},{"@language":"en","@value":"Chemical evolution of protoplanetary disks: the effect of dust evolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1041130850998983040","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"20H05847"},{"@type":"JGN","@value":"JP20H05847"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-20H05847/"}],"notation":[{"@language":"ja","@value":"気相・固相の反応素過程に基づく中間温度における分子進化モデル"},{"@language":"en","@value":"Theoretical astrochemistry based on microscopic processes in the gas and solid phases"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050584940308950016","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Evidence for Jet/Outflow Shocks Heating the Environment around the Class I Protostellar Source Elias 29: FAUST XXI"}]},{"@id":"https://cir.nii.ac.jp/crid/1050857822170401152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Cosmic-Ray Ionization Rate in Protoplanetary Disks with Sheared Magnetic Fields"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216959744640","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Growth efficiency of dust aggregates through collisions with high mass ratios"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217413772288","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Water in Star-forming Regions with the<i>Herschel Space Observatory</i>(WISH). I. Overview of Key Program and First Results"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217423697792","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHEMICAL PROCESSES IN PROTOPLANETARY DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004239676939392","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dust Continuum Emission and the Upper Limit Fluxes of Submillimeter Water Lines of the Protoplanetary Disk around HD 163296 Observed by ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143821019136","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry in disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143872965888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MEASURING PROTOPLANETARY DISK ACCRETION WITH H I PFUND β"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143974626560","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Highly structured disk around the planet host PDS 70 revealed by high-angular resolution observations with ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144234828928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gas Density Perturbations Induced by One or More Forming Planets in the AS 209 Protoplanetary Disk as Seen with ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144859042560","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Disk Substructures at High Angular Resolution Project (DSHARP). I. Motivation, Sample, Calibration, and Overview"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144981138688","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for unseen companions around T Tauri stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145027993344","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Resolving the inner dust disks surrounding LkCa 15  and MWC 480 at mm wavelengths"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145069495552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DETECTION OF N\n                    <sub>2</sub>\n                    D\n                    <sup>+</sup>\n                    IN A PROTOPLANETARY DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145561640960","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"VOLATILE DEPLETION IN THE TW HYDRAE DISK ATMOSPHERE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145640785280","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"PROTOPLANETARY DISK STRUCTURES IN OPHIUCHUS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146040304768","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry in disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146368953728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Physics of Dust Coagulation and the Structure of Dust Aggregates in Space"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146419992576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ALMA continuum observations of the protoplanetary disk AS 209"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168743992064","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"High Spatial Resolution Observations of Molecular Lines toward the Protoplanetary Disk around TW Hya with ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168798610432","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). III. Characteristics of Radial Chemical Substructures"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168798675328","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XIX. Spiral Arms, a Tail, and Diffuse Structures Traced by CO around the GM Aur Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168798705920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). IX. Distribution and Properties of the Large Organic Molecules HC<sub>3</sub>N, CH<sub>3</sub>CN, and c-C<sub>3</sub>H<sub>2</sub>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013168798724224","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). V. CO Gas Distributions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013171641812992","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The TW Hya Rosetta Stone Project. III. Resolving the Gaseous Thermal Profile of the Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013171659962880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-ray radiative transfer in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013171675518208","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Disk Illumination and Jet Variability of the Herbig Ae Star HD 163296 Using Multi-epoch HST/STIS Optical, Near-IR, and Radio Imagery and Spectroscopy"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013171767889664","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Constraining the Nature of the PDS 70 Protoplanets with VLTI/GRAVITY\n                  <sup>∗</sup>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013171818039040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Survey of C<sub>2</sub>H, HCN, and C<sup>18</sup>O in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013171960912256","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The ALMA Lupus protoplanetary disk survey: evidence for compact gas disks and molecular rings from CN"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172007535616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Modeling the nonaxisymmetric structure in the HD 163296 disk with planet-disk interaction"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172028762752","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). VIII. CO Gap in AS 209—Gas Depletion or Chemical Processing?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172074158464","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Interpreting high spatial resolution line observations of planet-forming disks with gaps and rings: the case of HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172252527488","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Chemical Inventory of the Planet-hosting Disk PDS 70"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172290477312","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Temperature Gradient in the Solar Nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172405270400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-ray emission from classical T Tauri stars: accretion shocks and coronae?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172543501312","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Case of Simultaneous Star and Planet Formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172573792512","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Bright C<sub>2</sub>H emission in protoplanetary discs in Lupus: high volatile C/O > 1 ratios"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013172797090944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"GoFish: Fishing for Line Observations in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013173024543232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"High resolution observations of molecular emission lines toward the CI Tau proto-planetary disc: planet-carved gaps or shadowing?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360013173202253440","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemical Evolution in a Protoplanetary Disk within Planet Carved Gaps and Dust Rings"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017279841326080","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Formation of Dust Clumps with Sub-Jupiter Mass and Cold Shadowed Region in Gravitationally Unstable Disk around Class 0/I Protostar in L1527 IRS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360017282436021248","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS): A Circumplanetary Disk Candidate in Molecular-line Emission in the AS 209 Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025429445837568","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. XII. Weighing and Sizing exoALMA Disks with Rotation Curve Modelling"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025429445927552","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. II. Data Calibration and Imaging Pipeline"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430629561088","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"MAPS: Constraining Serendipitous Time Variability in Protoplanetary Disk Molecular Ion Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692449021824","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A RECENT ACCRETION BURST IN THE LOW-MASS PROTOSTAR IRAS 15398-3359: ALMA IMAGING OF ITS RELATED CHEMISTRY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283692449143680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MASS ESTIMATES OF A GIANT PLANET IN A PROTOPLANETARY DISK FROM THE GAP STRUCTURES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283695761235456","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An ALMA Survey of DCN/H<sup>13</sup>CN and DCO<sup>+</sup>/H<sup>13</sup>CO<sup>+</sup> in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283695761864576","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Multiple Paths of Deuterium Fractionation in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360283695762737792","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"FIRST DETECTION OF GAS-PHASE METHANOL IN A PROTOPLANETARY DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285714653212032","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Flared Gas Structure of the Transitional Disk around Sz 91"}]},{"@id":"https://cir.nii.ac.jp/crid/1360287144383413376","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The First Detection of <sup>13</sup>C<sup>17</sup>O in a Protoplanetary Disk: A Robust Tracer of Disk Gas Mass"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292618721961472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Circumstellar material associated with solar-type pre-main-sequence stars - A possible constraint on the timescale for planet building"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292618786033152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Lupus disks with faint CO isotopologues: low gas/dust or high carbon depletion?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619038257152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"EVIDENCE FOR A CO DESORPTION FRONT IN THE OUTER AS 209 DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619040347008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Planet Shadows in Protoplanetary Disks. I. Temperature Perturbations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619257806720","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Evolution of Dust Disk Sizes from a Homogeneous Analysis of 1–10 Myr old Stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619484122880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MASS MEASUREMENTS IN PROTOPLANETARY DISKS FROM HYDROGEN DEUTERIDE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619581993856","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The<i>SPITZER</i>c2d Survey of Weak‐Line T Tauri Stars. I. Initial Results"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620091795072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHEMISTRY IN DISKS. III. PHOTOCHEMISTRY AND X-RAY DRIVEN CHEMISTRY PROBED BY THE ETHYNYL RADICAL (CCH) IN DM Tau, LkCa 15, AND MWC 480"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294646487346560","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Systematic Variations of CO Gas Abundance with Radius in Gas-rich Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294646625071744","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ionization-driven Depletion and Redistribution of CO in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294646789028480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The asymmetric inner disk of the Herbig Ae star HD 163296 in the eyes of VLTI/MATISSE: evidence for a vortex?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294646809426304","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The accretion rates and mechanisms of Herbig Ae/Be stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647108146304","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Masses and Implications for Ages of Low-mass Pre-main-sequence Stars in Taurus and Ophiuchus"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647147558784","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observational Signatures of Planets in Protoplanetary Disks: Planet-induced Line Broadening in Gaps"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647595819008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Connecting planet formation and astrochemistry"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647767007360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nitrile versus isonitrile adsorption at interstellar grains surfaces"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647826584576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observations of Protoplanetary Disk Structures"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647894745472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Investigating the Relative Gas and Small Dust Grain Surface Heights in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647937203840","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Sulfur Chemistry in Protoplanetary Disks: CS and H<sub>2</sub>CS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294647992871424","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ALMA detection of the rotating molecular disk wind from the young star HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294648076567552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Effects of Protostellar Disk Turbulence on CO Emission Lines: A Comparison Study of Disks with Constant CO Abundance versus Chemically Evolving Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294648191400320","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ingredients for solar-like systems: protostar IRAS 16293-2422 B versus comet 67P/Churyumov–Gerasimenko"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298754808965888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"FAUST"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302864775095936","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The First Spatially Resolved Detection of <sup>13</sup>CN in a Protoplanetary Disk and Evidence for Complex Carbon Isotope Fractionation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302866838305536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Kinematic signatures of a low-mass planet with a moderately inclined orbit in a protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302866863234816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"An Efficient Algorithm for Astrochemical Systems Using Stoichiometry Matrices"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306904415668864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"PDRs4All"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905176881920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Carbon-chain chemistry in the interstellar medium"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905643044864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. VI. Rotating under Pressure: Rotation Curves, Azimuthal Velocity Substructures, and Gas Pressure Variations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360306905643168768","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. I. Science Goals, Project Design, and Data Products"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565166913098496","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Unveiling the gas-and-dust disk structure in HD 163296 using ALMA observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182137735296","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Meridional circulation of gas into gaps opened by giant planets in three-dimensional low-viscosity disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574093756881024","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Two-dimensional distributions and column densities of gaseous\n molecules in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094756788224","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ALMA imaging of the CO snowline of the HD 163296 disk with DCO<sup>+</sup>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094976483456","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Modeling water emission from low-mass protostellar envelopes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095089075328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>HERSCHEL</i>EVIDENCE FOR DISK FLATTENING OR GAS DEPLETION IN TRANSITIONAL DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095256688512","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nine Localized Deviations from Keplerian Rotation in the DSHARP Circumstellar Disks: Kinematic Evidence for Protoplanets Carving the Gaps"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095333610496","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Evolution of Viscous Discs and the Origin of the Nebular Variables"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095356315264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry in protoplanetary disks: the gas-phase CO/H<sub>2</sub>ratio and the carbon reservoir"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095754570112","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A<i>SPITZER</i>SURVEY OF MID-INFRARED MOLECULAR EMISSION FROM PROTOPLANETARY DISKS. I. DETECTION RATES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096462949888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A<i>SPITZER</i>SURVEY OF MID-INFRARED MOLECULAR EMISSION FROM PROTOPLANETARY DISKS. II. CORRELATIONS AND LOCAL THERMAL EQUILIBRIUM MODELS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118752032256","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). VII. Substellar O/H and C/H and Superstellar C/O in Planet-feeding Gas"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118752068864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XI. CN and HCN as Tracers of Photochemistry in Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118752091264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). X. Studying Deuteration at High Angular Resolution toward Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118752150912","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XII. Inferring the C/O and S/H Ratios in Protoplanetary Disks with Sulfur Molecules"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576120170095872","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spiral Arms and a Massive Dust Disk with Non-Keplerian Kinematics: Possible Evidence for Gravitational Instability in the Disk of Elias 2–27"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576121560581760","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Flying Saucer:   Tomography of the thermal and density gas structure   of an edge-on protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576121867812096","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales. XX. The Massive Disk around GM Aurigae"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122087634048","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Submillimeter measurements of T Tauri and FU Orionis stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122127773440","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Robustness of N<sub>2</sub>H<sup>+</sup>as tracer of the CO snowline"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122130339328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Constraining Gas-phase Carbon, Oxygen, and Nitrogen in the IM Lup Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122139929600","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XVIII. Kinematic Substructures in the Disks of HD 163296 and MWC 480"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122625616000","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Role of C/O in Nitrile Astrochemistry in PDRs and Planet-forming Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576122954499200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spiral Structure in the Gas Disk of TW Hya"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576123069295104","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Three-phase Approach to Grain Surface Chemistry in Protoplanetary Disks: Gas, Ice Surfaces, and Ice Mantles of Dust Grains"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576123128154880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"AB Aur, a Rosetta stone for studies of planet formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576123135603200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemically tracing the water snowline in protoplanetary disks with HCO<sup>+</sup>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576123142555008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Ophiuchus DIsc Survey Employing ALMA (ODISEA) – III. The evolution of substructures in massive discs at 3–5 au resolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576123158671232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ring structure in the MWC 480 disk revealed by ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230594207360","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Architecture of Planetary Systems Predicted from Protoplanetary Disks Observed with ALMA. II. Evolution Outcomes and Dynamical Stability"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230610031232","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"CO Line Emission Surfaces and Vertical Structure in Midinclination Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580230610203136","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Mapping Protoplanetary Disk Vertical Structure with CO Isotopologue Line Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580232161679360","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Vibrationally Excited Lines of HC<sub>3</sub>N Associated with the Molecular Disk around the G24.78+0.08 A1 Hypercompact H ii Region"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584339771924352","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Early Planet Formation in Embedded Disks (eDisk). VIII. A Small Protostellar Disk around the Extremely Low Mass and Young Class 0 Protostar IRAS 15398–3359"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340513362176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Formation and Evolution Mechanisms for Organic Matter in Space"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584340513871616","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"An ALMA Molecular Inventory of Warm Herbig Ae Disks. I. Molecular Rings, Asymmetries, and Complexity in the HD 100546 Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360584341829659520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Early Planet Formation in Embedded Disks (eDisk). IV. The Ringed and Warped Structure of the Disk around the Class I Protostar L1489 IRS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588379373030784","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cloud Dissipation and Disk Wind in the Late Phase of Star Formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380164880000","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. XV. Interpreting the Height of CO Emission Layer"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588380164910976","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. XIII. Gas Masses from N<sub>2</sub>H<sup>+</sup> and C<sup>18</sup>O: A Comparison of Measurement Techniques for Protoplanetary Gas Disk Masses"}]},{"@id":"https://cir.nii.ac.jp/crid/1360588381082891904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"exoALMA. XIV. Gas Surface Densities in the RX J1604.3−2130 A Disk from Pressure-broadened CO Line Wings"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846641729286144","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The comet-like composition of a protoplanetary disk as revealed by complex cyanides"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846641889897216","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Complex organic molecules in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846642355901184","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DOUBLE DCO<sup>+</sup>RINGS REVEAL CO ICE DESORPTION IN THE OUTER DISK AROUND IM LUP"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659311539200","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"HIGH-CONTRAST NEAR-INFRARED POLARIZATION IMAGING OF MWC480"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855567865741440","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Matplotlib: A 2D Graphics Environment"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568419161344","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Rapid formation of Jupiter by diffusive redistribution of water vapor in the solar nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568491251712","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CO destruction in protoplanetary disk midplanes: Inside versus outside the CO snow surface"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568765312256","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Accretion Disks around Young Objects. II. Tests of Well‐mixed Models with ISM Dust"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569114227072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RESOLVING THE CO SNOW LINE IN THE DISK AROUND HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569356589184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE IMPRINT OF EXOPLANET FORMATION HISTORY ON OBSERVABLE PRESENT-DAY SPECTRA OF HOT JUPITERS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569401273984","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Warm H<sub>2</sub>O and OH in the disk around the Herbig star HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569601751168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"2018 Census of Interstellar, Circumstellar, Extragalactic, Protoplanetary Disk, and Exoplanetary Molecules"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569620956672","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569638675328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Cologne Database for Molecular Spectroscopy, CDMS: a useful tool for astronomers and spectroscopists"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569918014592","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Temperature Structures of Embedded Disks: Young Disks in Taurus Are Warm"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569940105088","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A protostellar system fed by a streamer of 10,500 au length"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569997871360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Warm molecular layers in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570467430144","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Origin of the RNA world: The fate of nucleobases in warm little ponds"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570691866752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ALMA chemical survey of disk-outflow sources in Taurus (ALMA-DOT)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571024179072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Disks around T Tauri Stars with SPHERE (DARTTS-S). I. SPHERE/IRDIS Polarimetric Imaging of Eight Prominent T Tauri Disks*"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593728713856","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). II. CLEAN Strategies for Synthesizing Images of Molecular Line Emission in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593728726656","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XV. Tracing Protoplanetary Disk Structure within 20 au"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593728750336","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). IV. Emission Surfaces and Vertical Distribution of Molecules"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593728785024","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XIII. HCO<sup>+</sup> and Disk Ionization Structure"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593728834688","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XVII. Determining the 2D Thermal Structure of the HD 163296 Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593728860032","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XVI. Characterizing the Impact of the Molecular Wind on the Evolution of the HD 163296 System"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857596603926912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Search for Spatially Resolved Infrared Rovibrational Molecular Hydrogen Emission from the Disks of Young Stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857596736235008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"HCO<sup>+</sup> DETECTION OF DUST-DEPLETED GAS IN THE INNER HOLE OF THE LkCa 15 PRE-TRANSITIONAL DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597169408384","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An ALMA Survey of H<sub>2</sub>CO in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597201137408","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Observational Constraints on Transport (and Mixing) in Pre-Main Sequence Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597289281792","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for a Cosmic-Ray Gradient in the IM Lup Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597292357632","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). XIV. Revealing Disk Substructures in Multiwavelength Continuum Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597358971904","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry Along Accretion Streams in a Viscously Evolving Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597709231488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references","isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Molecules with ALMA at Planet-forming Scales (MAPS). VI. Distribution of the Small Organics HCN, C<sub>2</sub>H, and H<sub>2</sub>CO"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597773605504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mass constraints for 15 protoplanetary discs from HD 1–0"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597935779328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The TW Hya Rosetta Stone Project. I. Radial and Vertical Distributions of DCN and DCO<sup>+</sup>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857597978498688","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for a Vertical Dependence on the Pressure Structure in AS 209"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857598067657728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An Unbiased ALMA Spectral Survey of the LkCa 15 and MWC 480 Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857598103353088","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A three-dimensional view of Gomez’s hamburger"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857598190642432","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Imaging the water snowline in a protostellar envelope with H<sup>13</sup>CO<sup>+</sup>"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857598200433024","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The chemistry of disks around T Tauri and Herbig Ae/Be stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861705563659648","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Sulphur monoxide emission tracing an embedded planet in the HD 100546 protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1360861705571352576","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The Molecular Composition of Shadowed Proto-solar Disk Midplanes Beyond the Water Snowline"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869855123419904","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Support for fragile porous dust in a gravitationally self-regulated disk around IM Lup"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869855561834112","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"FAUST"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869856045162624","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Detection of Dimethyl Ether in the Central Region of the MWC 480 Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044431725440","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044777229312","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Three-dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk Using DCO<sup>+</sup>"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044966209920","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A spectroscopic survey of Herbig Ae/Be stars with X-shooter – I. Stellar parameters and accretion rates"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045292974336","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Formation, Orbital and Internal Evolutions of Young Planetary Systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046088943232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Radiation thermo-chemical models of protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046222347392","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The outcome of protoplanetary dust growth: pebbles, boulders, or planetesimals?"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046234061184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Disk Substructures at High Angular Resolution Project (DSHARP). IX. A High-definition Study of the HD 163296 Planet-forming Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046456029056","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"USING FUV TO IR VARIABILITY TO PROBE THE STAR–DISK CONNECTION IN THE TRANSITIONAL DISK OF GM AUR"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046464807424","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE DISK IMAGING SURVEY OF CHEMISTRY WITH SMA. I. TAURUS PROTOPLANETARY DISK DATA"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518392981632","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gas modelling in the disc of HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518509135232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The NumPy Array: A Structure for Efficient Numerical Computation"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518572086656","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing the structure of protoplanetary disks: a comparative study of DM Tau, LkCa 15, and MWC 480"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518648625408","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An atomic and molecular database for analysis of submillimetre line observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518763720960","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Investigating grain growth in disks around southern T Tauri stars   at millimetre wavelengths"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518823138944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Excess C/H in Protoplanetary Disk Gas from Icy Pebble Drift Across the CO Snowline"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519268056576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ALMA unveils rings and gaps in the protoplanetary system HD 169142: signatures of two giant protoplanets"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519397002112","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Gas Temperature in the Surface Layers of Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519737190016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gas-Phase CO in Protoplanetary Disks: A Challenge for Turbulent Mixing"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519830780032","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ringed Structures of the HD 163296 Protoplanetary Disk Revealed by ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519898763264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Direct imaging of extra-solar planets in star forming regions"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520549475712","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Kinematic Evidence for an Embedded Protoplanet in a Circumstellar Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520861559936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An old disk still capable of forming a planetary system"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521159522688","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE STICKINESS OF MICROMETER-SIZED WATER-ICE PARTICLES"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521168462336","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Multifrequency ALMA Characterization of Substructures in the GM Aur Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521263193728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"EXPLORING THE ORIGINS OF DEUTERIUM ENRICHMENTS IN SOLAR NEBULAR ORGANICS"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699993680554624","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X‐Ray Ionization of Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699993882336128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Forming Planets via Pebble Accretion"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994118568064","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A SPATIALLY RESOLVED INNER HOLE IN THE DISK AROUND GM AURIGAE"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994143916800","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing dust grain evolution in IM Lupi's circumstellar disc"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994400576000","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Organic molecules in protoplanetary disks around T Tauri and Herbig Ae stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994712609792","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet–Disk Interactions Interpretation"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994744650368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Radiation thermo-chemical models of protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699996037187584","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Survey of CH<sub>3</sub>CN and HC<sub>3</sub>N in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699996295550336","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Chemistry of Multiply Deuterated Molecules in Protoplanetary Disks. I. The Outer Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981468566709888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"EVIDENCE FOR MULTIPLE PATHWAYS TO DEUTERIUM ENHANCEMENTS IN PROTOPLANETARY DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981468696484608","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RINGED SUBSTRUCTURE AND A GAP AT 1 au IN THE NEAREST PROTOPLANETARY DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981469241758848","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Effects of Dust Growth and Settling in T Tauri Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981469613235840","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Chemical Composition of Comets—Emerging Taxonomies and Natal Heritage"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981469833984896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry in disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470088521728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Millimeter imaging of HD 163296: probing the disk structure   and\n kinematics"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470162553216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Relating jet structure to photometric variability: the Herbig Ae star HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981471253462784","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Cometary Chemistry and the Origin of Icy Solar System Bodies: The View After Rosetta"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943740620928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Subarcsecond ALMA Molecular Line Imaging Survey of the Circumbinary, Protoplanetary Disk Orbiting V4046 Sgr"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943900937472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Consistent dust and gas models for protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944247885440","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Binary Companions of Evolved Stars in APOGEE DR14: Search Method and Catalog of ∼5000 Companions"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944310934528","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ice condensation as a planet formation mechanism"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945003154432","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Testing the theory of grain growth and fragmentation by millimeter observations of protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945281628288","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DEUTERIUM CHEMISTRY IN PROTOPLANETARY DISKS. II. THE INNER 30 AU"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945288525696","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-ray and Molecular Emission from the Nearest Region of Recent Star Formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945552025472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Parameters of Herbig Ae/Be and Vega-type stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945714143616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Photoprocesses in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262945903996928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Structure of the DM Tau Outer Disk: Probing the vertical\nkinetic temperature gradient"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262946060134016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Submillimeter lines from circumstellar disks around pre-main\nsequence stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262946171044992","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Resolved gas cavities in transitional disks inferred from CO isotopologs with ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262946203523968","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemical tracers of episodic accretion in low-mass protostars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262946257489280","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Rings and Gaps in Protoplanetary Disks: Planets or Snowlines?"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262946342509568","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"KINEMATICS OF THE CO GAS IN THE INNER REGIONS OF THE TW Hya DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418317067904","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>HERSCHEL</i>/PACS SURVEY OF PROTOPLANETARY DISKS IN TAURUS/AURIGA—OBSERVATIONS OF [O I] AND [C II], AND FAR-INFRARED CONTINUUM"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418448320384","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418617285248","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gas and Dust Emission at the Outer Edge of Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418637184256","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dust Density Distribution and Imaging Analysis of Different Ice Lines in Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418803059584","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A KINETIC DATABASE FOR ASTROCHEMISTRY (KIDA)"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418807413504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Survey of Cold Water Lines in Protoplanetary Disks: Indications of Systematic Volatile Depletion"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419490634368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"New Constraints From Dust Lines on the Surface Densities of Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419500449408","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The ancient heritage of water ice in the solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419718491008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Synthesis of activated pyrimidine ribonucleotides in prebiotically plausible conditions"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419830139648","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"High Resolution Neutral Hydrogen Observations of the Barred Spiral Galaxy NGC 1365"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420326727168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CO Depletion in Protoplanetary Disks: A Unified Picture Combining Physical Sequestration and Chemical Processing"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420437545728","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gaps, rings, and non-axisymmetric structures in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420499244928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DISK IMAGING SURVEY OF CHEMISTRY WITH SMA. II. SOUTHERN SKY PROTOPLANETARY DISK DATA AND FULL SAMPLE STATISTICS"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420614606208","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Formation of the Giant Planets by Concurrent Accretion of Solids and Gas"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420727883776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Distribution and Excitation of CH<sub>3</sub>CN in a Solar Nebula Analog"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420922274944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE 2014 ALMA LONG BASELINE CAMPAIGN: FIRST RESULTS FROM HIGH ANGULAR RESOLUTION OBSERVATIONS TOWARD THE HL TAU REGION"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544421220040576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Determining protoplanetary disk gas masses from CO isotopologues line observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893621370880","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemistry in disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893702343168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Accretion onto Pre-Main-Sequence Stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893783760256","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHEMISTRY OF A PROTOPLANETARY DISK WITH GRAIN SETTLING AND Lyα RADIATION"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893982499968","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The evolution of the water distribution in a viscous protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894180758272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Detecting Weak Spectral Lines in Interferometric Data through Matched Filtering"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894551722752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Cavities in inner disks: the GM Aurigae case"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894780704896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE RADIAL DISTRIBUTION OF H<sub>2</sub> AND CO IN TW HYA AS REVEALED BY RESOLVED ALMA OBSERVATIONS OF CO ISOTOPOLOGUES"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894788522368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Methanol and its Relation to the Water Snowline in the Disk around the Young Outbursting Star V883 Ori"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894924315776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Kinematical Detection of Two Embedded Jupiter-mass Planets in HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894942134144","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"UNVEILING THE STRUCTURE OF PRE-TRANSITIONAL DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895324834816","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Disks in Transition in the Taurus Population:\n                    <i>Spitzer</i>\n                    IRS Spectra of GM Aurigae and DM Tauri"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895388092032","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Rotating Gaseous Disk around the T Tauri Star GM Aurigae"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825896029934976","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A break in the gas and dust surface density of the disc   around\n the T Tauri star IM Lupi"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825896272078464","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE STRUCTURE OF THE EVOLVED CIRCUMBINARY DISK AROUND V4046 Sgr"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825896387799936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CONSTRAINTS ON THE RADIAL VARIATION OF GRAIN GROWTH IN THE AS 209 CIRCUMSTELLAR DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368303343488","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Binding energies: New values and impact on the efficiency of chemical desorption"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368382263552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Cologne Database for Molecular Spectroscopy, CDMS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368667467520","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Disk Substructures at High Angular Resolution Project (DSHARP). III. Spiral Structures in the Millimeter Continuum of the Elias 27, IM Lup, and WaOph 6 Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368783952000","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Gas Mass Tracers in Protoplanetary Disks: CO is Still the Best"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369069408640","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Cologne Database for Molecular Spectroscopy, CDMS, in the Virtual Atomic and Molecular Data Centre, VAMDC"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369326733824","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Imaging of the CO Snow Line in a Solar Nebula Analog"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369372696576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE COUPLED PHYSICAL STRUCTURE OF GAS AND DUST IN THE IM Lup PROTOPLANETARY DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369686058496","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-shooter spectroscopy of young stellar objects in Lupus"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370145634048","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Upper limits on CH<sub>3</sub>OH in the HD 163296 protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843386254208","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Disk Substructures at High Angular Resolution Project (DSHARP). II. Characteristics of Annular Substructures"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843430606848","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A SIGNIFICANTLY LOW CO ABUNDANCE TOWARD THE TW Hya PROTOPLANETARY DISK: A PATH TO ACTIVE CARBON CHEMISTRY?"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843825918848","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"EXCLUSION OF COSMIC RAYS IN PROTOPLANETARY DISKS. II. CHEMICAL GRADIENTS AND OBSERVATIONAL SIGNATURES"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843863763968","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Disk Evolution, Element Abundances and Cloud Properties of Young Gas Giant Planets"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844368099328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHEMICAL EVOLUTION OF TURBULENT PROTOPLANETARY DISKS AND THE SOLAR NEBULA"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844777380736","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"INDIRECT DETECTION OF FORMING PROTOPLANETS VIA CHEMICAL ASYMMETRIES IN DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845032284160","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>Gaia</i> Data Release 2"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845776710912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing midplane CO abundance and gas temperature with DCO<sup>+</sup>\nin the protoplanetary disk around HD 169142"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845919480320","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dust modeling of the combined ALMA and SPHERE datasets of HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388846164988800","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"PLANET FORMATION SIGNPOSTS: OBSERVABILITY OF CIRCUMPLANETARY DISKS VIA GAS KINEMATICS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388846216072576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CN rings in full protoplanetary disks around young stars   as probes of disk structure"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388846229679104","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Multiwavelength analysis for interferometric (sub-)mm observations of protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388846318727808","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Direct mapping of the temperature and velocity gradients in discs"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388846350520448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Inferring giant planets from ALMA millimeter continuum and line observations in (transition) disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670318367676032","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mass inventory of the giant-planet formation zone in a solar nebula analogue"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670318528777344","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CYANIDE PHOTOCHEMISTRY AND NITROGEN FRACTIONATION IN THE MWC 480 DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319387734272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemical and Thermal Structure of Protoplanetary Disks as Observed with ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319468279936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CO and Dust Properties in the TW Hya Disk from High-resolution ALMA Observations"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319634874496","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE COEVALITY OF YOUNG BINARY SYSTEMS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319682638976","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Far-ultraviolet and X-ray irradiated protoplanetary disks: a grid of models"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319826115968","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHEMICAL IMAGING OF THE CO SNOW LINE IN THE HD 163296 DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319984263808","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Unlocking CO Depletion in Protoplanetary Disks. I. The Warm Molecular Layer"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670320447913600","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Polarized Disk Emission from Herbig Ae/Be Stars Observed Using Gemini Planet Imager: HD 144432, HD 150193, HD 163296, and HD 169142"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670320537652736","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE DEPLETION OF WATER DURING DISPERSAL OF PLANET-FORMING DISK REGIONS"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793331965824","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Probing CO and N<sub>2</sub> Snow Surfaces in Protoplanetary Disks with N<sub>2</sub>H<sup>+</sup> Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793434948480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Meridional flows in the disk around a young star"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793498165376","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The HH30 edge-on T Tauri star"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793706780928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Effects of UV Continuum and Ly Radiation on the Chemical Equilibrium of T Tauri Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795390499072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Disk Substructures at High Angular Resolution Program (DSHARP). VIII. The Rich Ringed Substructures in the AS 209 Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795551353472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Resolving the Chemistry in the Disk of TW Hydrae. I. Deuterated Species"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795829992448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DCO<sup>+</sup>, DCN, and N<sub>2</sub>D<sup>+</sup>reveal three different deuteration regimes in the disk around the Herbig Ae star HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795846899456","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Astrochemistry and compositions of planetary systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268166040576","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A PARAMETRIC MODELING APPROACH TO MEASURING THE GAS MASSES OF CIRCUMSTELLAR DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268187910912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Common origins of RNA, protein and lipid precursors in a cyanosulfidic protometabolism"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268861179648","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ACCRETION VARIABILITY OF HERBIG Ae/Be STARS OBSERVED BY X-SHOOTER HD 31648 AND HD 163296"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269336859136","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The chemistry of episodic accretion in embedded objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269661718528","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"WEAK TURBULENCE IN THE HD 163296 PROTOPLANETARY DISK REVEALED BY ALMA CO OBSERVATIONS"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269823967232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE ROLE OF ICE COMPOSITIONS FOR SNOWLINES AND THE C/N/O RATIOS IN ACTIVE DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269829349376","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Multiple Rings in the Transitional Disk of GM Aurigae Revealed by VLA and ALMA"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269836430336","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"HYDROCARBON EMISSION RINGS IN PROTOPLANETARY DISKS INDUCED BY DUST EVOLUTION"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269882672896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SUBMILLIMETER, MILLIMETER, AND MICROWAVE SPECTRAL LINE CATALOG"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270486336640","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Can grain growth explain transition disks?"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270582319744","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Molecular Hydrogen Emission from Protoplanetary Disks. II. Effects of X‐Ray Irradiation and Dust Evolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270917297536","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE EFFECTS OF SNOWLINES ON C/O IN PLANETARY ATMOSPHERES"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233271159449600","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mid-IR spectra of pre-main sequence Herbig stars: An explanation for the non-detections of water lines"}]},{"@id":"https://cir.nii.ac.jp/crid/1370017669088490368","@type":"Product","relationType":["references"]},{"@id":"https://cir.nii.ac.jp/crid/1521136280363888896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Structure of the Solar Nebula,Growth and Decay of Magnetic Fields and Effects of Magnetic and Turbulent Viscosities on the Nebula"},{"@language":"ja-Kana","@value":"Structure of the Solar Nebula Growth an"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1432"},{"@type":"KAKEN","@value":"PRODUCT-24703950"},{"@type":"KAKEN","@value":"PRODUCT-24106020"},{"@type":"KAKEN","@value":"PRODUCT-23954304"},{"@type":"KAKEN","@value":"PRODUCT-24618994"},{"@type":"KAKEN","@value":"PRODUCT-24624355"},{"@type":"OPENAIRE","@value":"doi_dedup___::a176311e53657c67db58a3e050d249c1"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1434_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac143e_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1441_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1580_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac794e_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1431_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/ac86c2_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac22ae_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/ac7fa3_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adc431_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adc43a_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/acf315_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202243414_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad2fb4_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1093/pasj/psad059_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ad12c8_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202450988_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/adabe7_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1007/s10509-024-04292-9_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adb152_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adc43b_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1435_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac143a_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac143d_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac2583_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac68de_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1440_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac6c02_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/acb3c4_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac69d1_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad003a_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.2138/gselements.20.1.13_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-3881/ad2700_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/accd71_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad4997_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adc42e_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adc430_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/adc42f_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1430_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1433_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1439_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac143c_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac143f_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1ad4_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202244472_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ac87fa_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac1438_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4365/ac143b_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1038/s41550-024-02308-6_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/202450742_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ad6981_references_DOI_1OXgUtWUO2caYeESzidEniREbMy"}]}