{"@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/1360286994656299520.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1093/pasj/psz069"}},{"identifier":{"@type":"URI","@value":"https://academic.oup.com/pasj/article-pdf/71/4/87/54667252/pasj_71_4_87.pdf"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1905.11897"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Spectropolarimetry of the superwind filaments of the starburst galaxy M 82 II: Kinematics of the dust surrounding the nuclear starburst"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title>\n               <jats:p>We performed deep spectropolarimetric observations of the prototypical starburst galaxy M 82 with the Subaru Telescope in order to study the kinematics of the dust outflow. We obtained optical polarized emission-line spectra up to ∼4 kpc away from the nucleus of the galaxy along three position angles, 138°, 150°, and 179° within the conical outflowing wind (superwind). The Hα emission line in the superwind is strongly polarized and the polarization pattern shows dust scattering of central light sources, being consistent with the previous works. The intensity weighted polarization degree of the Hα line reaches ∼30% at maximum. There are at least two light sources at the central region of the galaxy; one is located at the near-infrared nucleus and the other resides at one of the peaks of the 3 mm radio and molecular gas emission. The outer (&gt;1 kpc) dust is illuminated by the former, whereas the inner dust is scattering the light from the latter. We also investigated the dust motion from the velocity field of the polarized Hα emission line. The dust is accelerated outward on the northwest side of the nucleus. A simple bi-conical dust outflow model shows that the outflow velocity of the dust reaches ≳ 300–450 km s−1 at ∼4 kpc from the nucleus, suggesting that some portion of the dust escapes from the gravitational potential of M 82 into the intergalactic space. At some regions on the southeast side, in particular along the position angle of 138°, the dust has a radial velocity that is slower than the systemic velocity of the galaxy, apparently suggesting inflowing motion toward the nucleus. These components are spatially consistent with a part of the molecular gas stream, which is kinematically independent of the outflow gas; thus the apparent inflow motion of the dust reflects the streaming motion associated with the molecular gas stream.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1420564276179253120","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"90270446"},{"@type":"NRID","@value":"1000090270446"},{"@type":"NRID","@value":"9000017708717"},{"@type":"NRID","@value":"9000006447157"},{"@type":"NRID","@value":"9000239608676"},{"@type":"NRID","@value":"9000242546871"},{"@type":"NRID","@value":"9000267810164"},{"@type":"NRID","@value":"9000009495279"},{"@type":"NRID","@value":"9000399527256"},{"@type":"NRID","@value":"9000267810150"},{"@type":"NRID","@value":"9000000123029"},{"@type":"NRID","@value":"9000239608859"},{"@type":"NRID","@value":"9000239608825"},{"@type":"NRID","@value":"9000410920522"},{"@type":"NRID","@value":"9000009904606"},{"@type":"NRID","@value":"9000009495269"},{"@type":"NRID","@value":"9000248219249"},{"@type":"NRID","@value":"9000248219236"},{"@type":"NRID","@value":"9000244902290"},{"@type":"NRID","@value":"9000322675978"},{"@type":"NRID","@value":"9000331897763"},{"@type":"NRID","@value":"9000267810159"},{"@type":"NRID","@value":"9000267805249"},{"@type":"NRID","@value":"9000267810165"},{"@type":"NRID","@value":"9000398834536"},{"@type":"NRID","@value":"9000009917493"},{"@type":"NRID","@value":"9000408879813"},{"@type":"NRID","@value":"9000408879819"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/read0187649"}],"foaf:name":[{"@value":"Michitoshi Yoshida"}],"jpcoar:affiliationName":[{"@value":"Subaru Telescope, National Astronomical Observatory of Japan, 650 North A’ohoku Place, Hilo, HI 96720, USA"},{"@value":"Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380286994656299404","@type":"Researcher","foaf:name":[{"@value":"Koji S Kawabata"}],"jpcoar:affiliationName":[{"@value":"Hiroshima Astrophysical Science Center, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380286994656299907","@type":"Researcher","foaf:name":[{"@value":"Youichi Ohyama"}],"jpcoar:affiliationName":[{"@value":"Academia Sinica, Institute of Astronomy and Astrophysics, 11F of AS/NTU, Astronomy-Mathematics Building, No. 1, Sec. 4, Roosevelt Rd., Taipei 10617, Taiwan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380286994656299271","@type":"Researcher","foaf:name":[{"@value":"Ryosuke Itoh"}],"jpcoar:affiliationName":[{"@value":"Department of Physical Science, Hiroshima University, 1-3-1 Kagamiyama, Higashi-Hiroshima, Hiroshima 739-8526, Japan"},{"@value":"Department of Physics, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan"}]},{"@id":"https://cir.nii.ac.jp/crid/1380286994656299654","@type":"Researcher","foaf:name":[{"@value":"Takashi Hattori"}],"jpcoar:affiliationName":[{"@value":"Subaru Telescope, National Astronomical Observatory of Japan, 650 North A’ohoku Place, Hilo, HI 96720, USA"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00046264"},{"@type":"EISSN","@value":"2053051X"}],"prism:publicationName":[{"@value":"Publications of the Astronomical Society of Japan"}],"dc:publisher":[{"@value":"Oxford University Press (OUP)"}],"prism:publicationDate":"2019-08-01","prism:volume":"71","prism:number":"4","prism:startingPage":"87"},"reviewed":"false","dcterms:accessRights":"http://purl.org/coar/access_right/c_abf2","dc:rights":["http://creativecommons.org/licenses/by/4.0/"],"url":[{"@id":"https://academic.oup.com/pasj/article-pdf/71/4/87/54667252/pasj_71_4_87.pdf"}],"createdAt":"2019-06-04","modifiedAt":"2023-12-20","foaf:topic":[{"@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=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Astrophysics%20of%20Galaxies","dc:title":"Astrophysics - Astrophysics of Galaxies"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781825079552","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15H02069"},{"@type":"JGN","@value":"JP15H02069"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-15H02069/"}],"notation":[{"@language":"ja","@value":"可視近赤外線同時偏光観測によるガンマ線バーストの研究"},{"@language":"en","@value":"Study of gamma-ray bursts with optical near-infrared simultaneous polarimetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781959601024","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06363"},{"@type":"JGN","@value":"JP17H06363"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-17H06363/"}],"notation":[{"@language":"ja","@value":"重力波源の光赤外線対応天体観測で迫る中性子星合体の元素合成"},{"@language":"en","@value":"Study of nucleosynthesis in neutron star merger with optical-infrared follow-up observations of gravitational wave sources"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781959608576","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06357"},{"@type":"JGN","@value":"JP17H06357"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-ORGANIZER-17H06357/"}],"notation":[{"@language":"ja","@value":"重力波物理学・天文学：創世記(総括班)"},{"@language":"en","@value":"Gravitational wave physics and astronomy: Genesis"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360004233709117952","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Large-scale distributions of mid- and far-infrared emission from the center to the halo of M 82 revealed with AKARI"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144199705088","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Starburst at the Expanding Molecular Superbubble in M82: Self‐induced Starburst at the Inner Edge of the Superbubble"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144217942784","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DEMOGRAPHICS AND PHYSICAL PROPERTIES OF GAS OUTFLOWS/INFLOWS AT 0.4 <<i>z</i>< 1.4"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145239510656","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spectroscopic FIR mapping of the disk and galactic wind of M 82 with<i>Herschel</i>-PACS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146009880064","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Infrared mapping of M82 - A starburst in an edge-on barred galaxy"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617498005504","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Hydrogen recombination near-infrared line mapping of Centaurus A with IRSF/SIRIUS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619402726400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"NEUTRAL HYDROGEN CLOUDS IN THE M81/M82 GROUP"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619974076032","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Absorption‐Line Probes of Gas and Dust in Galactic Superwinds"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620289597184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Infrared imaging and polarimetry of M82 - Evidence for a ring of warm dust"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620481185024","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565167604102400","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Large-Field CO (<i>J</i> = 1→0) Observations of the Starburst Galaxy M 82"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574093974034944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"MAXIMALLY STAR-FORMING GALACTIC DISKS. I. STARBURST REGULATION VIA FEEDBACK-DRIVEN TURBULENCE"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094834634496","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>GALEX</i>\n                    Observations of the Ultraviolet Halos of NGC 253 and M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095075540352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Nature of Starburst Activity in M821"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095986338176","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"FOCAS: The Faint Object Camera and Spectrograph for the Subaru Telescope"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096008566400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Three‐Dimensional Simulations of a Starburst‐driven Galactic Wind"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096016676096","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The scattered H  emission-line filaments in M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096173136896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RADIATION FEEDBACK IN ULIRGs: ARE PHOTONS MOVERS AND SHAKERS?"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096352753920","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Large-scale bipolar wind in M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096476139008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Grisms Developed for FOCAS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096573023488","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE ORIGIN AND KINEMATICS OF COLD GAS IN GALACTIC WINDS: INSIGHT FROM NUMERICAL SIMULATIONS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568943895424","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"EXTENDED HCN AND HCO<sup>+</sup>EMISSION IN THE STARBURST GALAXY M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571039368448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"High-resolution X-ray imaging of the Starburst Galaxy M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869855116723200","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"What Are the Radial Distributions of Density, Outflow Rates, and Cloud Structures in the M82 Wind?"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044680617600","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Properties of FOCAS optical components"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045819487360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Extended Mid-Infrared Aromatic Feature Emission in M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046446948992","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518766260224","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Detection of the Red Giant Branch Stars in M82 Using the<i>Hubble Space Telescope</i>"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518922548736","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DIRECT NUMERICAL SIMULATION OF RADIATION PRESSURE-DRIVEN TURBULENCE AND WINDS IN STAR CLUSTERS AND GALACTIC DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519320219776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Wind from a starburst galaxy nucleus"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519834485888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The spectral energy distribution of CO lines in M 82"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521399492352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Numerical simulations of radiatively driven dusty winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994030723584","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"DUST SCATTERING AND THE RADIATION PRESSURE FORCE IN THE M82 SUPERWIND"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994650572416","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Feedback-regulated star formation in molecular clouds and galactic discs"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994922413184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A New Spectropolarimeter at the Dodaira Observatory"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995397217280","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mapping Large‐Scale Gaseous Outflows in Ultraluminous Galaxies with Keck II ESI Spectra: Variations in Outflow Velocity with Galactic Mass"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995719028864","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"X-Ray Spectral Study of the Extended Emission, ‘the Cap’, Located 11.6 kpc above the Disk of M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699996116723328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dynamics of dusty radiation-pressure-driven shells and clouds: fast outflows from galaxies, star clusters, massive stars, and AGN"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981468675504640","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dynamics and X-ray emission of a galactic superwind interacting with disk and halo gas"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981468955343744","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A High Spatial Resolution X‐Ray and Hα Study of Hot Gas in the Halos of Star‐forming Disk Galaxies. I. Spatial and Spectral Properties of the Diffuse X‐Ray Emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981468979784064","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for large-scale winds from starburst galaxies. I - The nature of the ionized gas in M82 and NGC 253"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470196587520","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chandra High-Resolution Camera observations of the luminous X-ray source in the starburst galaxy M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470400678656","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"On the nature and implications of starburst-driven galactic superwinds"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470618539008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Superbubble blowout dynamics"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981471297258240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Current Performance and On-Going Improvements of the 8.2 m Subaru Telescope"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943587523328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"RADIATION PRESSURE FROM MASSIVE STAR CLUSTERS AS A LAUNCHING MECHANISM FOR SUPER-GALACTIC WINDS"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943799453568","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spatially resolved Spitzer-IRS spectral maps of the superwind in M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944279638912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Molecular Gas in M82: Resolving the Outflow and Streamers"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418454586368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Outflows in Infrared‐Luminous Starbursts at\n                    <i>z</i>\n                    < 0.5. II. Analysis and Discussion"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419015236480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"WARM MOLECULAR HYDROGEN IN THE GALACTIC WIND OF M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420393985152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SCALING RELATIONS BETWEEN WARM GALACTIC OUTFLOWS AND THEIR HOST GALAXIES"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420740735360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE MOLECULAR BARYON CYCLE OF M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420921980800","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Radiation Hydrodynamic Simulations of Dust-driven Winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544421067818368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>Hubble Space Telescope</i>Advanced Camera for Surveys Mosaic of the Prototypical Starburst Galaxy M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544421161127808","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"First-look XMM-Newton EPIC observations of the prototypical starburst galaxy M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894739092864","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Astronomical Polarimetry"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894861333376","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Decomposition of the Superwind in M 82"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895150830720","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evolution of dust grains through a hot gaseous halo"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895440749952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The biconical kiloparsec structure generated by nuclear starbursts"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895633885696","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Magnetized gas clouds can survive acceleration by a hot wind"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368359849600","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Galactic Winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368944207616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE MULTI-PHASE COLD FOUNTAIN IN M82 REVEALED BY A WIDE, SENSITIVE MAP OF THE MOLECULAR INTERSTELLAR MEDIUM"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369240823424","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Constraints on star formation driven galaxy winds from the mass-metallicity relation at z= 0"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369515129216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Starburst-driven galactic winds -- I. Energetics and intrinsic X-ray emission"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369860945408","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A high-resolution image of atomic hydrogen in the M81 group of galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843224012672","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Asymmetric Wind in M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843765571328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Discovery of a Luminous, Variable, Off-Center Source in the Nucleus of M82 with the [ITAL]Chandra[/ITAL] High-Resolution Camera"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844032009856","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"H I streamers around M82 - Tidally disrupted outer gas disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845120984832","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Metal Enrichment of the Intergalactic Medium at<i>z</i> = 3 by Galactic Winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845263472896","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SUBMILLIMETER CONTINUUM PROPERTIES OF COLD DUST IN THE INNER DISK AND OUTFLOWS OF M 82"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845293198976","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"H i Kinematics along the Minor Axis of M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845564086272","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Stellar feedback in galaxies and the origin of galaxy-scale winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670318367699968","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"BLACK HOLE POWERED NEBULAE AND A CASE STUDY OF THE ULTRALUMINOUS X-RAY SOURCE IC 342 X-1"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319639849088","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Spectropolarimetry of the Superwind Filaments of the Starburst Galaxy M 82: Kinematics of Dust Outflow"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319820730752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The rotating visible outflow in M 82"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319859962240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The First Light of the Subaru Telescope: A New Infrared Image of the Orion Nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319955832192","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dusty Cloud Acceleration by Radiation Pressure in Rapidly Star-forming Galaxies"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793521752960","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<i>Light Scattering by Small Particles</i>"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793652532096","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE OPTICAL STRUCTURE OF THE STARBURST GALAXY M82. II. NEBULAR PROPERTIES OF THE DISK AND INNER WIND"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951794791459072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Sub-Eddington star-forming regions are super-Eddington: momentum-driven outflows from supersonic turbulence"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795898003200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Enrichment of the Intergalactic Medium by Radiation Pressure–driven Dust Efflux"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268596756992","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"LARGE HIGHLY IONIZED NEBULAE AROUND ULTRA-LUMINOUS X-RAY SOURCES"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268600747008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"SUPERNOVA FEEDBACK EFFICIENCY AND MASS LOADING IN THE STARBURST AND GALACTIC SUPERWIND EXEMPLAR M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268606819456","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Galaxies and Intergalactic Matter at Redshift<i>z</i> ∼ 3: Overview"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268688272640","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"THE SYSTEMATIC PROPERTIES OF THE WARM PHASE OF STARBURST-DRIVEN GALACTIC WINDS"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268852530432","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The peculiar dust distribution of M82"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269381166720","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemical footprint of star formation feedback in M 82 on scales of ~100 pc"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269900500480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An ultraluminous X-ray source powered by an accreting neutron star"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1093/pasj/psz069"},{"@type":"KAKEN","@value":"PRODUCT-23414260"},{"@type":"KAKEN","@value":"PRODUCT-22839439"},{"@type":"KAKEN","@value":"PRODUCT-22872524"},{"@type":"OPENAIRE","@value":"doi_dedup___::7fc2eabbc3c966fc449bf19173f9d706"},{"@type":"CROSSREF","@value":"10.1093/pasj/psaa081_references_DOI_RheI5AvyaHjDpjxao7BeQuH0o7I"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/acfa71_references_DOI_RheI5AvyaHjDpjxao7BeQuH0o7I"}]}