Mass-loss Processes
Mass-Loss Processes is a theoretical construct in stellar astrophysics that refers to the mechanisms by which pre-main sequence stars eject material from their outer layers through winds, jets, and disk outflows, thereby reducing their mass during early evolutionary stages.
1.3K
Publications
88.8K
Citations
3.3K
Authors
920
Institutions
Publications per year
2017–2026
264
Parents
1.3K
Dynamics of the Interplanetary Gas and Magnetic Fields.
E. N. Parker · The Astrophysical Journal · 1958 · 3.6K citations
Natural Sciences, Astronomy, Physics +17
Mass-loss predictions for O and B stars as a function of metallicity
Astronomy and Astrophysics · 2001 · 1.7K citations · Full text
Natural Sciences, Astronomy, Physics +17
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
39 h-index
143 publications
8.9K citations
University of California, Berkeley
Berkeley, United States
33 h-index
93 publications
7.3K citations

Centre National de la Recherche Scientifique
Paris, France
33 h-index
197 publications
14.9K citations
California Institute of Technology
Pasadena, United States
33 h-index
135 publications
14.5K citations
Goddard Space Flight Center
Greenbelt, United States
32 h-index
100 publications
6.5K citations

University of Amsterdam
Amsterdam, The Netherlands
31 h-index
101 publications
10.2K citations
KU Leuven
Leuven, Belgium
31 h-index
151 publications
7.6K citations
The University of Tokyo
Tokyo, Japan
29 h-index
86 publications
5.1K citations
1–8 of 920
ApJ · 420 publications · 35.2K citations
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190 publications · 15K citations
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233 publications · 15.1K citations
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AJ · 36 publications · 1.7K citations
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Repository · 30 publications · 1.9K citations
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