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On the Stability and Evolution of Isolated Molecular Clouds

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dc.contributor.author Langer, W. en_US
dc.contributor.author Nelson, R. en_US
dc.date.accessioned 2004-09-25T17:32:16Z
dc.date.available 2004-09-25T17:32:16Z
dc.date.issued 1998
dc.identifier.citation Astrophysical Journal en_US
dc.identifier.clearanceno 98-1760
dc.identifier.uri http://hdl.handle.net/2014/20703
dc.description.abstract We 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. en_US
dc.format.extent 1850204 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other interstellor clouds hydrodynamics molecular clouds star formation thermal pressure chemical evolution interstellar radiation en_US
dc.title On the Stability and Evolution of Isolated Molecular Clouds en_US


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