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Massive Infrared-Quiet Dense Cores: Unveiling the Initial Conditions of High-Mass Star Formation

hal.structure.identifierDépartement d'Astrophysique, de physique des Particules, de physique Nucléaire et de l'Instrumentation Associée [DAPNIA]
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorMOTTE, F.
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire Hétérochimie Fondamentale et Appliquée [LHFA]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorBONTEMPS, Sylvain
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
hal.structure.identifierCEREG [CEREG]
hal.structure.identifierDepartment of Health Sciences Research [Mayo Clinic] [HSR]
hal.structure.identifierAntarctic Research a European Network for Astrophysics [ARENA]
dc.contributor.authorSCHNEIDER, N.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorSCHILKE, P.
hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
dc.contributor.authorMENTEN, K. M.
dc.date.created2008
dc.date.issued2008
dc.date.conference2007-09-10
dc.description.abstractEnAs Th. Henning said at the conference, cold precursors of high-mass stars are now ''hot topics''. We here propose some observational criteria to identify massive infrared-quiet dense cores which can host the high-mass analogs of Class~0 protostars and pre-stellar condensations. We also show how far-infrared to millimeter imaging surveys of entire complexes forming OB stars are starting to unveil the initial conditions of high-mass star formation.
dc.language.isoen
dc.source.titleMassive Star Formation: Observations Confront Theory ASP Conference Series, Vol. 387
dc.title.enMassive Infrared-Quiet Dense Cores: Unveiling the Initial Conditions of High-Mass Star Formation
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.identifier.arxiv0801.1636
bordeaux.page22
bordeaux.volume387
bordeaux.conference.titleproceedings of the conference held 10-14 September 2007 at Heidelberg Convention Center, Heidelberg, Germany. Edited by Henrik Beuther, Hendrik Linz, and Thomas Henning. San Francisco: Astronomical Society of the Pacific, 2008
bordeaux.countryDE
bordeaux.title.proceedingMassive Star Formation: Observations Confront Theory ASP Conference Series, Vol. 387
bordeaux.conference.cityHeidelberg
bordeaux.peerReviewedoui
hal.identifierhal-00203614
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00203614v1
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