Stellar Spin-up

Stellar Spin-Up is a theoretical construct in astrophysics that denotes the process by which a star increases its angular velocity due to the conservation of angular momentum during gravitational contraction or mass accretion.

127

Publications

10.1K

Citations

336

Authors

229

Institutions

Publications per year

2017–2026

41

Variants

Stellar Spin Up

Authors

336

  1. JF
    Jim Fuller

    California Institute of Technology, United States

    3 publications · 407 citations

    3

    h-index

  2. SS
    Sergey S. Tsygankov

    University of Turku, Finland

    3 publications · 117 citations

    3

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    3 publications · 375 citations

    3

    h-index

  4. SP
    Sean P. Matt

    University of Exeter, United Kingdom

    3 publications · 133 citations

    3

    h-index

  5. JW
    J. Wilms

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    3 publications · 92 citations

    3

    h-index

1–5 of 336

Venues

  1. The Astrophysical Journal

    ApJ · 48 publications · 5K citations

    34

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    22 publications · 1.5K citations

    17

    h-index

  3. Astronomy and Astrophysics

    15 publications · 636 citations

    15

    h-index

  4. The Astrophysical Journal Letters

    6 publications · 491 citations

    6

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 3 publications · 63 citations

    3

    h-index

1–5