NASA NTRS · 19880021153
Star formation and molecular clouds
Abstract
Several differnt stages can be discerned within the star formation process. Star formation can be considered to start when a molecular cloud fragments into many clumps. Many different physical processes are likely to play an important role in star formation, including self-gravity, magnetic fields, rotation, winds, and radiation transport. The current knowledge on some of these processes are reviewed.
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Tielens, Alexander G. G. M.. 1988-01-01. Star formation and molecular clouds. https://ntrs.nasa.gov/citations/19880021153
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