{"@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/1363388844231163776.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1093/mnras/stz3336"}},{"identifier":{"@type":"URI","@value":"http://academic.oup.com/mnras/article-pdf/492/1/1180/31784582/stz3336.pdf"}}],"dc:title":[{"@value":"ALMA and ROSINA detections of phosphorus-bearing molecules: the interstellar thread between star-forming regions and comets"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>ABSTRACT</jats:title>\n               <jats:p>To understand how phosphorus (P)-bearing molecules are formed in star-forming regions, we have analysed the Atacama Large Millimeter/Submillimeter Array (ALMA) observations of PN and PO towards the massive star-forming region AFGL 5142, combined with a new analysis of the data of the comet 67P/Churyumov–Gerasimenko taken with the Rosetta Orbiter Spectrometer for Ion and Neutral Analysis (ROSINA) instrument onboard Rosetta. The ALMA maps show that the emission of PN and PO arises from several spots associated with low-velocity gas with narrow linewidths in the cavity walls of a bipolar outflow. PO is more abundant than PN in most of the spots, with the PO/PN ratio increasing as a function of the distance to the protostar. Our data favour a formation scenario in which shocks sputter phosphorus from the surface of dust grains, and gas-phase photochemistry induced by UV photons from the protostar allows efficient formation of the two species in the cavity walls. Our analysis of the ROSINA data has revealed that PO is the main carrier of P in the comet, with PO/PN &gt; 10. Since comets may have delivered a significant amount of prebiotic material to the early Earth, this finding suggests that PO could contribute significantly to the phosphorus reservoir during the dawn of our planet. There is evidence that PO was already in the cometary ices prior to the birth of the Sun, so the chemical budget of the comet might be inherited from the natal environment of the Solar system, which is thought to be a stellar cluster including also massive stars.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1383388844231163780","@type":"Researcher","foaf:name":[{"@value":"V M Rivilla"}],"jpcoar:affiliationName":[{"@value":"INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125, Florence, Italy"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163906","@type":"Researcher","foaf:name":[{"@value":"M N Drozdovskaya"}],"jpcoar:affiliationName":[{"@value":"Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, CH-3012 Bern, Switzerland"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163788","@type":"Researcher","foaf:name":[{"@value":"K Altwegg"}],"jpcoar:affiliationName":[{"@value":"Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163783","@type":"Researcher","foaf:name":[{"@value":"P Caselli"}],"jpcoar:affiliationName":[{"@value":"Max-Planck-Institute for Extraterrestrial Physics, Garching, 85741, Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163793","@type":"Researcher","foaf:name":[{"@value":"M T Beltrán"}],"jpcoar:affiliationName":[{"@value":"INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125, Florence, Italy"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163790","@type":"Researcher","foaf:name":[{"@value":"F Fontani"}],"jpcoar:affiliationName":[{"@value":"INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125, Florence, Italy"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163787","@type":"Researcher","foaf:name":[{"@value":"F F S van der Tak"}],"jpcoar:affiliationName":[{"@value":"SRON Netherlands Institute for Space Research, Landleven 12, NL-9747 AD Groningen, the Netherlands"},{"@value":"Kapteyn Astronomical Institute, University of Groningen, 9747 AD, Groningen, the Netherlands"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163779","@type":"Researcher","foaf:name":[{"@value":"R Cesaroni"}],"jpcoar:affiliationName":[{"@value":"INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125, Florence, Italy"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163778","@type":"Researcher","foaf:name":[{"@value":"A Vasyunin"}],"jpcoar:affiliationName":[{"@value":"Ural Federal University, Ekaterinburg, 620002, Russia"},{"@value":"Visiting Leading Researcher, Engineering Research Institute ‘Ventspils International Radio Astronomy Centre’ of Ventspils University of Applied Sciences, Inženieru 101, Ventspils LV-3601, Latvia"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163781","@type":"Researcher","foaf:name":[{"@value":"M Rubin"}],"jpcoar:affiliationName":[{"@value":"Center for Space and Habitability, University of Bern, Gesellschaftsstrasse 6, CH-3012 Bern, Switzerland"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163786","@type":"Researcher","foaf:name":[{"@value":"F Lique"}],"jpcoar:affiliationName":[{"@value":"LOMC, UMR 6294, CNRS-Université du Havre, France"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163776","@type":"Researcher","foaf:name":[{"@value":"S Marinakis"}],"jpcoar:affiliationName":[{"@value":"School of Health, Sport and Bioscience, University of East London, Stratford Campus, Water Lane, London E15 4LZ, UK"},{"@value":"Department of Chemistry and Biochemistry, School of Biological and Chemical Sciences, Queen Mary University of London, Joseph Priestley Building, Mile End Road, London E1 4NS, UK"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163785","@type":"Researcher","foaf:name":[{"@value":"L Testi"}],"jpcoar:affiliationName":[{"@value":"INAF-Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, I-50125, Florence, Italy"},{"@value":"ESO/European Southern Observatory, Karl Schwarzschild str. 2, D-85748, Garching, Germany"},{"@value":"Excellence Cluster ‘Universe’, Boltzmann str. 2, D-85748 Garching bei Muenchen, Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163782","@type":"Researcher","foaf:name":[{"@value":"H Balsiger"}],"jpcoar:affiliationName":[{"@value":"Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163784","@type":"Researcher","foaf:name":[{"@value":"J J Berthelier"}],"jpcoar:affiliationName":[{"@value":"LATMOS, 4 Avenue de Neptune, F-94100 SAINT-MAUR, France"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163905","@type":"Researcher","foaf:name":[{"@value":"J De Keyser"}],"jpcoar:affiliationName":[{"@value":"Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Ringlaan 3, B-1180 Brussels, Belgium"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163791","@type":"Researcher","foaf:name":[{"@value":"B Fiethe"}],"jpcoar:affiliationName":[{"@value":"Institute of Computer and Network Engineering (IDA), TU Braunschweig, Hans-Sommer-Strasse 66, D-38106 Braunschweig, Germany"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163792","@type":"Researcher","foaf:name":[{"@value":"S A Fuselier"}],"jpcoar:affiliationName":[{"@value":"Space Science Division, Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78228, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163904","@type":"Researcher","foaf:name":[{"@value":"S Gasc"}],"jpcoar:affiliationName":[{"@value":"Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163789","@type":"Researcher","foaf:name":[{"@value":"T I Gombosi"}],"jpcoar:affiliationName":[{"@value":"Department of Atmospheric, Oceanic and Space Sciences, University of Michigan, 2455 Hayward, Ann Arbor, MI 48109, USA"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163777","@type":"Researcher","foaf:name":[{"@value":"T Sémon"}],"jpcoar:affiliationName":[{"@value":"Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland"}]},{"@id":"https://cir.nii.ac.jp/crid/1383388844231163794","@type":"Researcher","foaf:name":[{"@value":"C-Y Tzou"}],"jpcoar:affiliationName":[{"@value":"Physikalisches Institut, University of Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00358711"},{"@type":"EISSN","@value":"13652966"}],"prism:publicationName":[{"@value":"Monthly Notices of the Royal Astronomical Society"}],"dc:publisher":[{"@value":"Oxford University Press (OUP)"}],"prism:publicationDate":"2020-01-15","prism:volume":"492","prism:number":"1","prism:startingPage":"1180","prism:endingPage":"1198"},"reviewed":"false","dc:rights":["https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model"],"url":[{"@id":"http://academic.oup.com/mnras/article-pdf/492/1/1180/31784582/stz3336.pdf"}],"createdAt":"2019-12-10","modifiedAt":"2020-01-15","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360013168740737920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Experimental and Computational Studies on the Physicochemical Behavior of Phosphine Induced by Reactions with H and D Atoms on Interstellar Ice Grains"}]},{"@id":"https://cir.nii.ac.jp/crid/1360021389814187008","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Reaction dynamics on amorphous solid 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