NASA NTRS · 20060041621
On the Stability and Evolution of Isolated Molecular Clouds
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.
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Langer, W., Nelson, R.. 1998-01-01. On the Stability and Evolution of Isolated Molecular Clouds. https://ntrs.nasa.gov/citations/20060041621
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