Mass Quenching
Mass quenching is a theoretical mechanism in galactic evolution wherein the cessation of star formation in a galaxy is primarily driven by its stellar mass, distinguishing it from environment-dependent quenching processes.
85
Publications
8.8K
Citations
488
Authors
238
Institutions
Publications per year
2017–2026
47
Parents
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488
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Centre National de la Recherche Scientifique
Paris, France
14 h-index
25 publications
3.1K citations
Laboratoire d’Astrophysique de Marseille
Marseille, France
11 h-index
29 publications
23.3K citations
Carnegie Observatories
Pasadena, United States
10 h-index
12 publications
769 citations
ETH Zurich
Zurich, Switzerland
9 h-index
31 publications
29.4K citations
University of California, Irvine
Irvine, United States
9 h-index
23 publications
2K citations
Osservatorio Astronomico di Padova
Padua, Italy
8 h-index
9 publications
3K citations
California Institute of Technology
Pasadena, United States
8 h-index
12 publications
2.9K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
8 h-index
10 publications
6.6K citations
1–8 of 238
38 publications · 3.5K citations
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ApJ · 17 publications · 3.3K citations
15
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9 publications · 548 citations
9
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2 publications · 202 citations
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Repository · 2 publications · 84 citations
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