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

Authors

518

  1. MS
    M. S. Chu

    General Atomics (United States), United States

    8 publications · 453 citations

    8

    h-index

  2. NL
    N. Langer

    University of Bonn, Germany

    6 publications · 510 citations

    6

    h-index

  3. SS
    S.A. Sabbagh

    Columbia University, United States

    5 publications · 356 citations

    5

    h-index

  4. RL
    R.J. La Haye

    General Atomics (United States), United States

    5 publications · 302 citations

    5

    h-index

  5. MO
    M. Okabayashi

    Princeton Plasma Physics Laboratory, United States

    5 publications · 319 citations

    5

    h-index

1–5 of 518

Venues

  1. The Astrophysical Journal

    ApJ · 24 publications · 1.7K citations

    20

    h-index

  2. Physical Review Letters

    PRL · 20 publications · 1.9K citations

    18

    h-index

  3. Astronomy and Astrophysics

    14 publications · 1.8K citations

    14

    h-index

  4. Physical Review A

    PRA · 12 publications · 572 citations

    12

    h-index

  5. 11

    h-index

1–5