Critical Rotation
Critical Rotation is a theoretical threshold in stellar astrophysics representing the maximum angular velocity at which a star can rotate without undergoing equatorial mass loss due to the balance between gravitational attraction and centrifugal force.
171
Publications
10.5K
Citations
518
Authors
270
Institutions
Publications per year
2017–2026
32
Parents
171
Nicola Pizzolato, A. Maggio, G. Micela et al. · Astronomy and Astrophysics · 2002 · 861 citations · Full text
Natural Sciences, Astronomy, Physics +14
Vortex Nucleation in a Stirred Bose-Einstein Condensate
Chandra Raman, J. R. Abo-Shaeer, J. M. Vogels et al. · Physical Review Letters · 2001 · 388 citations · Full text
Be-star rotation: how close to critical?
Monthly Notices of the Royal Astronomical Society · 2004 · 331 citations · Full text
Natural Sciences, Astronomy, Physics +14
A STELLAR ROTATION CENSUS OF B STARS: FROM ZAMS TO TAMS
Wenjin Huang, Douglas R. Gies, M. V. McSwain · The Astrophysical Journal · 2010 · 267 citations · Full text
Natural Sciences, Astronomy, Physics +16
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270

Centre National de la Recherche Scientifique
Paris, France
15 h-index
44 publications
2.2K citations
Columbia University
New York, United States
10 h-index
27 publications
2.1K citations
General Atomics (United States)
San Diego, United States
10 h-index
51 publications
3.5K citations

Princeton Plasma Physics Laboratory
Princeton, United States
10 h-index
37 publications
2.6K citations
University of Oxford
Oxford, United Kingdom
6 h-index
10 publications
860 citations
Chalmers University of Technology
Gothenburg, Sweden
6 h-index
9 publications
586 citations
University of Geneva
Geneva, Switzerland
6 h-index
13 publications
614 citations

Université Fédérale de Toulouse Midi-Pyrénées
Toulouse, France
6 h-index
18 publications
472 citations
1–8 of 270
ApJ · 24 publications · 1.7K citations
20
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PRL · 20 publications · 1.9K citations
18
h-index
14 publications · 1.8K citations
14
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PRA · 12 publications · 572 citations
12
h-index
11 publications · 727 citations
11
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