On the Stability and Evolution of Isolated Molecular Clouds

Langer, W.; Nelson, R.

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