Breakup Velocity
Breakup Velocity is the theoretical maximum rotational velocity at which a star would cease to hold itself together due to centrifugal forces balancing gravitational forces, leading to mass loss at the equator.
90
Publications
5.8K
Citations
279
Authors
148
Institutions
Publications per year
2017–2026
17
Variants
Critical Rotational VelocityKeplerian Velocity
Parents
90
NASA's new breakup model of evolve 4.0
Nicholas L. Johnson, Paula H. Krisko, J.‐C. Liou et al. · Advances in Space Research · 2001 · 391 citations
Rotational and radial velocities of T Tauri stars
Lee Hartmann, R. Hewett, Steven W. Stahler et al. · The Astrophysical Journal · 1986 · 253 citations
Natural Sciences, Astronomy, Physics +14
1–5 of 90
279
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Universitatea Națională de Știință și Tehnologie Politehnica București, Romania
2 publications · 31 citations
2
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2
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1–5 of 279
148

Centre National de la Recherche Scientifique
Paris, France
6 h-index
11 publications
922 citations

Kyoto University
Kyoto, Japan
4 h-index
6 publications
456 citations
Stony Brook University
Stony Brook, United States
3 h-index
3 publications
66 citations
Purdue University West Lafayette
West Lafayette, United States
3 h-index
9 publications
558 citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
2 h-index
2 publications
192 citations
CEA Paris-Saclay
Gif-sur-Yvette, France
2 h-index
2 publications
192 citations
Princeton University
Princeton, United States
2 h-index
6 publications
146 citations

United States Naval Research Laboratory
Washington, United States
2 h-index
5 publications
123 citations
1–8 of 148
ApJ · 13 publications · 886 citations
13
h-index
5 publications · 1.5K citations
5
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3 publications · 136 citations
3
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3 publications · 36 citations
3
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3 publications · 98 citations
3
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