The Dynamical Structure and Evolution of Giant Molecular Clouds

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dc.creatorMcKee, Christopher F.
dc.date1999-01-26
dc.date.accessioned2026-07-07T02:30:12Z
dc.date.available2026-07-07T02:30:12Z
dc.descriptionGiant molecular clouds (GMCs) are the sites of star formation in the Galaxy. Many of their properties can be understood in terms of a model in which the GMCs and the star-forming clumps within them are in approximate pressure equilibrium, with turbulent motions treated as a separate pressure component.
dc.description38 pages. Conference: The Physics of Star Formation and Early Stellar Evolution (Crete II)
dc.identifierhttps://arxiv.org/abs/astro-ph/9901370
dc.identifierhttp://arxiv.org/abs/astro-ph/9901370
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13741
dc.subjectAstrophysics
dc.titleThe Dynamical Structure and Evolution of Giant Molecular Clouds
dc.typetext

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