Stellar Spin-down

Stellar Spin-Down is a theoretical construct in stellar astrophysics that describes the gradual reduction in a star's angular velocity over time due to the loss of rotational angular momentum, primarily through magnetized stellar winds.

241

Publications

18K

Citations

775

Authors

353

Institutions

Publications per year

2017–2026

59

Variants

Stellar Spin Down

Authors

775

  1. SP
    Sean P. Matt

    University of Exeter, United Kingdom

    8 publications · 1K citations

    8

    h-index

  2. FC
    F. Camilo

    Columbia University, United States

    6 publications · 461 citations

    6

    h-index

  3. AT
    A. Tiengo

    Istituto di Astrofisica Spaziale e Fisica Cosmica di Milano, Italy

    5 publications · 208 citations

    5

    h-index

  4. DL
    Dong Lai

    Cornell University, United States

    5 publications · 479 citations

    5

    h-index

  5. RT
    R. Turolla

    University of Padua, Italy

    5 publications · 208 citations

    5

    h-index

1–5 of 775

Venues

  1. The Astrophysical Journal

    ApJ · 93 publications · 8.8K citations

    51

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    60 publications · 3.8K citations

    35

    h-index

  3. The Astrophysical Journal Letters

    13 publications · 870 citations

    13

    h-index

  4. Astronomy and Astrophysics

    13 publications · 386 citations

    12

    h-index

  5. CERN Document Server (European Organization for Nuclear Research)

    Repository · 7 publications · 831 citations

    7

    h-index

1–5