The Stellar Initial Mass Function from Turbulent Fragmentation
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/576/i=2/a=870/pdf
Reference131 articles.
1. A Theory of the Initial Mass Function for Star Formation in Molecular Clouds
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4. Interaction of proto-stars in a collapsing cluster
5. Turbulent Flow–driven Molecular Cloud Formation: A Solution to the Post–T Tauri Problem?
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