Stellar Mass Function Evolution
Stellar Mass Function Evolution is a theoretical construct in astrophysics that characterizes the time-dependent distribution of stellar masses within galaxies, distinguishing itself from static mass functions by explicitly modeling how the abundance of stars across different mass bins changes over cosmic time due to star formation, stellar evolution, and galaxy interactions.
349
Publications
51.8K
Citations
1.1K
Authors
412
Institutions
Publications per year
2017–2026
97
Parents
349
On the variation of the initial mass function
Pavel Kroupa · Monthly Notices of the Royal Astronomical Society · 2001 · 7.5K citations · Full text
Natural Sciences, Astronomy, Physics +16
The Galactic Center massive black hole and nuclear star cluster
R. Genzel, Frank Eisenhauer, S. Gillessen · Reviews of Modern Physics · 2010 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +16
1–5 of 349
1.1K
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412

Centre National de la Recherche Scientifique
Paris, France
32 h-index
171 publications
44.9K citations
Leiden University
Leiden, The Netherlands
24 h-index
41 publications
18.7K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
24 h-index
74 publications
14.1K citations
California Institute of Technology
Pasadena, United States
24 h-index
49 publications
11.1K citations

Durham University
Durham, United Kingdom
22 h-index
75 publications
60.3K citations
National Institute for Astrophysics
Rome, Italy
22 h-index
107 publications
13.4K citations
University of Bonn
Bonn, Germany
22 h-index
43 publications
4.6K citations
Institut d'Astrophysique de Paris
Paris, France
20 h-index
41 publications
9.9K citations
1–8 of 412
142 publications · 29.1K citations
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ApJ · 96 publications · 11.4K citations
53
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40 publications · 4.3K citations
30
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10 publications · 549 citations
9
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5 publications · 226 citations
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