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On the Stability and Evolution of Isolated Molecular CloudsWe present the results of three dimensional hydrodynamic models of evolving, isolated, low mass, quiescent clouds and Bok gobules, where the interstellar radiation field plays an important role in the thermal and chemical evolution, and thermal pressure provides dominant support against gravitational collapse.
Document ID
20060041621
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Langer, W.
Nelson, R.
Date Acquired
August 23, 2013
Publication Date
January 1, 1998
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
pressure chemical evolution interstellar radiation
interstellor clouds hydrodynamics molecular clouds star formation thermal

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