The Properties of Dense Molecular Gas in the Milky Way and Galaxies

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dc.creatorShirley, Yancy L.
dc.creatorWu, Jingwen
dc.creatorBussmann, R. Shane
dc.creatorWootten, Al
dc.date2007-11-28
dc.date.accessioned2026-07-07T08:45:57Z
dc.date.available2026-07-07T08:45:57Z
dc.descriptionWe review the evidence for a constant star formation rate per unit mass in dense molecular gas in the Milky Way and the extragalactic correlations of L_IR with L' from observations of dense molecular gas. We discuss the connection between the constant SFR/M interpretation in dense gas and the global Schmidt-Kennicutt star formation law.
dc.description7 pages. To appear in Massive Star Formation: Observations Confront Theory, ed. H. Beuther, ASP Conference Series
dc.identifierhttps://arxiv.org/abs/0711.4605
dc.identifierhttp://arxiv.org/abs/0711.4605
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/143128
dc.subjectAstrophysics
dc.titleThe Properties of Dense Molecular Gas in the Milky Way and Galaxies
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