Physical versus Observational Properties of Clouds in Turbulent Molecular Cloud Models
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/570/i=2/a=734/pdf
Reference44 articles.
1. Ambiguities in the identification of giant molecular cloud complexes from longitude-velocity diagrams
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4. Clouds as Turbulent Density Fluctuations: Implications for Pressure Confinement and Spectral Line Data Interpretation
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