Stellar Rotation Evolution
Stellar Rotation Evolution is a theoretical construct in astrophysics that describes the changes in a star's angular velocity during the pre-main-sequence phase, distinguishing itself from other stellar evolutionary processes by focusing specifically on the developmental trajectory of rotational dynamics under the influence of accretion, magnetic braking, and angular momentum redistribution.
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675
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2017–2026
210
Parents
951
Rotating massive main-sequence stars
I. Brott, S. E. de Mink, Matteo Cantiello et al. · Astronomy and Astrophysics · 2011 · 873 citations · Full text
Natural Sciences, Astronomy, Physics +15
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Centre National de la Recherche Scientifique
Paris, France
51 h-index
347 publications
22.4K citations
University of Geneva
Geneva, Switzerland
38 h-index
182 publications
14.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
38 h-index
129 publications
12K citations
Université Paris Cité
Paris, France
35 h-index
99 publications
9.7K citations
California Institute of Technology
Pasadena, United States
31 h-index
80 publications
6K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
29 h-index
72 publications
5.7K citations
Astrophysique, Instrumentation et Modélisation
Gif-sur-Yvette, France
28 h-index
68 publications
5.5K citations

Space Telescope Science Institute
Baltimore, United States
28 h-index
46 publications
4.2K citations
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ApJ · 298 publications · 24.4K citations
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196 publications · 15.1K citations
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132 publications · 7.3K citations
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AJ · 48 publications · 3.4K citations
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Repository · 30 publications · 1.9K citations
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