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

Authors

279

  1. JB
    J. Bouvier

    Centre National de la Recherche Scientifique, France

    2 publications · 59 citations

    2

    h-index

  2. JL
    J.‐C. Liou

    Johnson Space Center, United States

    2 publications · 403 citations

    2

    h-index

  3. PE
    Paul E. Sojka

    Purdue University West Lafayette, United States

    2 publications · 101 citations

    2

    h-index

  4. CB
    Corneliu Bălan

    Universitatea Națională de Știință și Tehnologie Politehnica București, Romania

    2 publications · 31 citations

    2

    h-index

  5. JC
    J. C. Wells

    Ritsumeikan University, Japan

    2 publications · 73 citations

    2

    h-index

1–5 of 279

Venues

  1. The Astrophysical Journal

    ApJ · 13 publications · 886 citations

    13

    h-index

  2. International Journal of Multiphase Flow

    5 publications · 1.5K citations

    5

    h-index

  3. Physics of Fluids

    3 publications · 136 citations

    3

    h-index

  4. Nuclear Physics A

    3 publications · 36 citations

    3

    h-index

  5. 3

    h-index

1–5