Main Sequence Rotation
Main Sequence Rotation is a theoretical construct in stellar astrophysics that characterizes the rotational evolution of low- to intermediate-mass stars during their stable hydrogen-burning phase on the main sequence, distinguishing it from pre-main-sequence and post-main-sequence rotational behaviors.
377
Publications
25.7K
Citations
922
Authors
409
Institutions
Publications per year
2017–2026
93
Parents
377
Rotation, convection, and magnetic activity in lower main-sequence stars
R. W. Noyes, Lee Hartmann, S. L. Baliunas et al. · The Astrophysical Journal · 1984 · 1.8K citations
Natural Sciences, Astronomy, Physics +14
The Progenitor Stars of Gamma‐Ray Bursts
S. E. Woosley, Alexander Heger · The Astrophysical Journal · 2006 · 941 citations · Full text
Natural Sciences, Astronomy, Physics +17
1–5 of 377
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Center for Astrophysics Harvard & Smithsonian, United States
10 publications · 2.9K citations
10
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9
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1–5 of 922
409

Centre National de la Recherche Scientifique
Paris, France
33 h-index
126 publications
6.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
70 publications
5.1K citations
University of Geneva
Geneva, Switzerland
22 h-index
67 publications
10.1K citations
Université Paris Cité
Paris, France
18 h-index
49 publications
2.4K citations

Université Fédérale de Toulouse Midi-Pyrénées
Toulouse, France
15 h-index
24 publications
1.8K citations

Space Telescope Science Institute
Baltimore, United States
15 h-index
37 publications
2K citations
Osservatorio Astronomico di Padova
Padua, Italy
14 h-index
23 publications
1K citations
The University of Tokyo
Tokyo, Japan
14 h-index
25 publications
2.9K citations
1–8 of 409
ApJ · 135 publications · 12K citations
57
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62 publications · 3.6K citations
36
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51 publications · 2.5K citations
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AJ · 24 publications · 1.3K citations
19
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PASP · 15 publications · 579 citations
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