Stellar Rotation Evolution

Stellar Rotation Evolution is a theoretical construct in astrophysics that describes the changes in a star's angular velocity during the pre-main-sequence phase, distinguishing itself from other stellar evolutionary processes by focusing specifically on the developmental trajectory of rotational dynamics under the influence of accretion, magnetic braking, and angular momentum redistribution.

951

Publications

68.1K

Citations

2K

Authors

675

Institutions

Publications per year

2017–2026

210

Authors

2K

  1. GM
    G. Meynet

    University of Geneva, Switzerland

    47 publications · 5K citations

    34

    h-index

  2. AM
    A. Maeder

    Global Social Observatory, Switzerland

    33 publications · 4.1K citations

    26

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    22 publications · 4K citations

    21

    h-index

  4. MH
    Marc H. Pinsonneault

    The Ohio State University, United States

    19 publications · 3.2K citations

    18

    h-index

  5. CC
    C. Charbonnel

    Centre National de la Recherche Scientifique, France

    21 publications · 1.9K citations

    18

    h-index

1–5 of 2K

Venues

  1. The Astrophysical Journal

    ApJ · 298 publications · 24.4K citations

    82

    h-index

  2. Astronomy and Astrophysics

    196 publications · 15.1K citations

    66

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    132 publications · 7.3K citations

    47

    h-index

  4. The Astronomical Journal

    AJ · 48 publications · 3.4K citations

    29

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 30 publications · 1.9K citations

    23

    h-index

1–5