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CO observations of the molecular gas in the Galactic H ii region Sh2-48: Evidence for cloud–cloud collision as a trigger of high-mass star formation

dc.contributor.authorTorii, Ken_US
dc.contributor.authorHattori, Yen_US
dc.contributor.authorMatsuo, Men_US
dc.contributor.authorFujita, Sen_US
dc.contributor.authorNishimura, Aen_US
dc.contributor.authorKohno, Men_US
dc.contributor.authorKuriki, Men_US
dc.contributor.authorTsuda, Yen_US
dc.contributor.authorMinamidani, Ten_US
dc.contributor.authorUmemoto, Ten_US
dc.contributor.authorKuno, Nen_US
dc.contributor.authorYoshiike, Sen_US
dc.contributor.authorOhama, Aen_US
dc.contributor.authorTachihara, Ken_US
dc.contributor.authorFukui, Yen_US
dc.contributor.authorShima, Ken_US
dc.contributor.authorHabe, Aen_US
dc.contributor.authorHaworth, TJen_US
dc.date.accessioned2019-11-01T13:21:38Z
dc.date.available2018-05-03en_US
dc.date.issued2018-10-31en_US
dc.identifier.issn0004-6264en_US
dc.identifier.urihttps://qmro.qmul.ac.uk/xmlui/handle/123456789/61078
dc.languageenen_US
dc.publisherOxford University Press (OUP)en_US
dc.relation.ispartofPublications of the Astronomical Society of Japanen_US
dc.titleCO observations of the molecular gas in the Galactic H ii region Sh2-48: Evidence for cloud–cloud collision as a trigger of high-mass star formationen_US
dc.typeArticle
dc.rights.holder© The Author(s) 2018. Published by Oxford University Press on behalf of the Astronomical Society of Japan.
dc.identifier.doi10.1093/pasj/psy098en_US
pubs.notesNot knownen_US
pubs.publication-statusPublisheden_US
dcterms.dateAccepted2018-05-03en_US
rioxxterms.funderDefault funderen_US
rioxxterms.identifier.projectDefault projecten_US


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