Stellar Angular Momentum

Stellar Angular Momentum is the rotational analogue of linear momentum in stars, defined as the product of a star's moment of inertia and its angular velocity, accounting for the distribution and motion of stellar mass about its axis of rotation.

1.3K

Publications

108.5K

Citations

2.6K

Authors

783

Institutions

Publications per year

2017–2026

293

Authors

2.6K

  1. SM
    S. Mathis

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    23 publications · 1.7K citations

    20

    h-index

  2. GM
    G. Meynet

    University of Geneva, Switzerland

    26 publications · 1.9K citations

    19

    h-index

  3. PE
    P. Eggenberger

    University of Geneva, Switzerland

    22 publications · 970 citations

    17

    h-index

  4. CC
    C. Charbonnel

    Centre National de la Recherche Scientifique, France

    18 publications · 934 citations

    16

    h-index

  5. AM
    A. Maeder

    Global Social Observatory, Switzerland

    17 publications · 1.6K citations

    16

    h-index

1–5 of 2.6K

Venues

  1. The Astrophysical Journal

    ApJ · 388 publications · 38.5K citations

    98

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    285 publications · 27.5K citations

    78

    h-index

  3. Astronomy and Astrophysics

    175 publications · 12K citations

    64

    h-index

  4. The Astronomical Journal

    AJ · 46 publications · 3.1K citations

    29

    h-index

  5. The Astrophysical Journal Letters

    33 publications · 2.6K citations

    24

    h-index

1–5