Rotational Mixing
Rotational Mixing is a stellar astrophysical process in which angular momentum and chemical elements are redistributed within a star due to rotation-induced hydrodynamic instabilities and shear flows, thereby modifying its internal composition and evolution.
290
Publications
21.3K
Citations
595
Authors
330
Institutions
Publications per year
2017–2026
43
290
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
The Evolution of Rotating Stars
Annual Review of Astronomy and Astrophysics · 2000 · 832 citations · Full text
Natural Sciences, Astronomy, Physics +17
Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes
P. G. Beck, J. Montalbán, T. Kallinger et al. · Nature · 2011 · 513 citations · Full text
Natural Sciences, Astronomy, Physics +16
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330
University of Geneva
Geneva, Switzerland
26 h-index
81 publications
8.7K citations

Centre National de la Recherche Scientifique
Paris, France
25 h-index
75 publications
6.9K citations
University of Bonn
Bonn, Germany
18 h-index
53 publications
8.4K citations
Utrecht University
Utrecht, The Netherlands
14 h-index
38 publications
8.5K citations
The University of Tokyo
Tokyo, Japan
12 h-index
16 publications
1.1K citations
Université Paris Cité
Paris, France
12 h-index
33 publications
3.3K citations

Space Telescope Science Institute
Baltimore, United States
12 h-index
22 publications
2.9K citations

University of Amsterdam
Amsterdam, The Netherlands
11 h-index
14 publications
2.6K citations
1–8 of 330
65 publications · 7.1K citations
41
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ApJ · 49 publications · 4.5K citations
31
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27 publications · 2.1K citations
22
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Repository · 14 publications · 1.1K citations
13
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Repository · 6 publications · 159 citations
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