Molecular Cloud Core Collapse
Molecular Cloud Core Collapse is a physical astrophysical process in protostellar evolution wherein a gravitationally unstable region within a molecular cloud undergoes contraction due to self-gravity, initiating the formation of a protostar by dissipating thermal and magnetic support mechanisms.
207
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17.8K
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234
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154
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2017–2026
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Toward Understanding Massive Star Formation
Annual Review of Astronomy and Astrophysics · 2007 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +16
The collapse of the cores of slowly rotating isothermal clouds
S. Terebey, Frank H. Shu, P. Cassen · The Astrophysical Journal · 1984 · 642 citations
Natural Sciences, Astronomy, Physics +16
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University of Exeter
Exeter, United Kingdom
14 h-index
20 publications
1.9K citations
Hosei University
Tokyo, Japan
12 h-index
12 publications
1.3K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
12 h-index
25 publications
2.9K citations

Carnegie Institution for Science
Washington, United States
12 h-index
16 publications
894 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
11 h-index
18 publications
1.3K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
10 h-index
18 publications
2.3K citations
Carnegie Observatories
Pasadena, United States
10 h-index
12 publications
751 citations
University of Chicago
Chicago, United States
8 h-index
12 publications
557 citations
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ApJ · 95 publications · 8.7K citations
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41 publications · 3.9K citations
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10 publications · 603 citations
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5 publications · 287 citations
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4 publications · 202 citations
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