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

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dc.creatorMotte, Frédérique
dc.creatorBontemps, S.
dc.creatorSchneider, N.
dc.creatorSchilke, P.
dc.creatorMenten, K. M.
dc.date2008-01-10
dc.date.accessioned2026-07-07T08:53:41Z
dc.date.available2026-07-07T08:53:41Z
dc.descriptionAs Pr. 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.identifierhttps://arxiv.org/abs/0801.1636
dc.identifierhttp://arxiv.org/abs/0801.1636
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/145709
dc.subjectAstrophysics
dc.titleMassive Infrared-Quiet Dense Cores: Unveiling the Initial Conditions of High-Mass Star Formation
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