Gas Expulsion is a theoretical construct in the study of clustered star formation that denotes the process by which residual molecular gas is dynamically removed from a young star cluster due to stellar feedback mechanisms such as radiation pressure, winds, and supernovae.
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436
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244
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2017–2026
48
Parents
Publications
171
1–5 of 171
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436
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16
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11
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9
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7
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6
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1–5 of 436
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244
University of Bonn
Bonn, Germany
23 h-index
49 publications
3.5K citations
University of Sheffield
Sheffield, United Kingdom
12 h-index
19 publications
2.1K citations
Centre National de la Recherche Scientifique
Paris, France
10 h-index
12 publications
950 citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
9 h-index
12 publications
596 citations
Institute of Astronomy
Moscow, Russia
9 h-index
14 publications
1.6K citations
Leiden University
Leiden, The Netherlands
9 h-index
19 publications
2K citations
Heidelberg University
Heidelberg, Germany
9 h-index
19 publications
1K citations
Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
8 h-index
10 publications
353 citations
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- Monthly Notices of the Royal Astronomical Society
48 publications · 4.2K citations
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- The Astrophysical Journal
ApJ · 20 publications · 1.2K citations
17
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- Astronomy and Astrophysics
16 publications · 907 citations
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- Nature
4 publications · 558 citations
4
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- The Astrophysical Journal Letters
4 publications · 193 citations
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