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Properties of the dense core population in Orion B as seen by the Herschel Gould Belt survey

hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
hal.structure.identifierJeremiah Horrocks Institute for Mathematics, Physics and Astronomy [Preston]
dc.contributor.authorKÖNYVES, V.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorANDRÉ, Ph.
hal.structure.identifierNagoya University
hal.structure.identifierInstituto de Astrofísica e Ciências do Espaço [IASTRO]
dc.contributor.authorARZOUMANIAN, D.
dc.contributor.authorSCHNEIDER, N.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorMEN’SHCHIKOV, A.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBONTEMPS, S.
hal.structure.identifierInstituto de RadioAstronomía Milimétrica [IRAM]
dc.contributor.authorLADJELATE, B.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorDIDELON, P.
hal.structure.identifierIstituto di Astrofisica e Planetologia Spaziali - INAF [IAPS]
dc.contributor.authorPEZZUTO, S.
hal.structure.identifierIstituto di Astrofisica e Planetologia Spaziali - INAF [IAPS]
dc.contributor.authorBENEDETTINI, M.
hal.structure.identifierAstrophysique
dc.contributor.authorBRACCO, A.
hal.structure.identifierNational Research Council of Canada [NRC]
hal.structure.identifierUniversity of Victoria [Canada] [UVIC]
dc.contributor.authorDI FRANCESCO, J.
hal.structure.identifierUniversity of Sheffield [Sheffield]
dc.contributor.authorGOODWIN, S.
hal.structure.identifierIstituto di Radioastronomia [Bologna] [IRA]
dc.contributor.authorRYGL, K. L. J.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorSHIMAJIRI, Y.
hal.structure.identifierIstituto di Astrofisica e Planetologia Spaziali - INAF [IAPS]
dc.contributor.authorSPINOGLIO, L.
hal.structure.identifierJeremiah Horrocks Institute for Mathematics, Physics and Astronomy [Preston]
dc.contributor.authorWARD-THOMPSON, D.
hal.structure.identifierSpace Science and Technology Department [Didcot] [RAL Space]
dc.contributor.authorWHITE, G. J.
dc.date.issued2020
dc.identifier.issn0004-6361
dc.description.sponsorshipVers une vision unifiée de la formation stellaire dans les galaxies : Origine de la structure filamentaire du milieu interstellaire, des cœurs pré-stellaires et des amas protostellaires vus avec Herschel
dc.description.sponsorshipGENeration et Evolution des Structures du milieu InterStellaire - ANR-16-CE92-0035
dc.language.isoen
dc.publisherEDP Sciences
dc.subject.ensubmillimeter: ISM
dc.subject.enISM: clouds
dc.subject.enstars: formation
dc.subject.enISM: individual objects: Orion B complex
dc.subject.enISM: structure
dc.subject.ensubmillimeter: ISM
dc.title.enProperties of the dense core population in Orion B as seen by the Herschel Gould Belt survey
dc.typeArticle de revue
dc.identifier.doi10.1051/0004-6361/201834753
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.identifier.arxiv1910.04053
dc.description.sponsorshipEuropeToward a Complete View of Star Formation: The Origin of Molecular Clouds, Prestellar Cores, and Star Clusters
dc.description.sponsorshipEuropeMastering the dusty and magnetized Interstellar Screen to Test Inflation Cosmology
bordeaux.journalAstronomy and Astrophysics - A&A
bordeaux.pageA34
bordeaux.volume635
bordeaux.peerReviewedoui
hal.identifiercea-02499010
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//cea-02499010v1
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