Main Sequence Rotation

Main Sequence Rotation is a theoretical construct in stellar astrophysics that characterizes the rotational evolution of low- to intermediate-mass stars during their stable hydrogen-burning phase on the main sequence, distinguishing it from pre-main-sequence and post-main-sequence rotational behaviors.

377

Publications

25.7K

Citations

922

Authors

409

Institutions

Publications per year

2017–2026

93

Authors

922

  1. CC
    C. Charbonnel

    Centre National de la Recherche Scientifique, France

    14 publications · 1.7K citations

    14

    h-index

  2. NB
    N. Bastian

    Liverpool John Moores University, United Kingdom

    10 publications · 553 citations

    10

    h-index

  3. JB
    J. Bouvier

    Centre National de la Recherche Scientifique, France

    10 publications · 404 citations

    10

    h-index

  4. LH
    Lee Hartmann

    Center for Astrophysics Harvard & Smithsonian, United States

    10 publications · 2.9K citations

    10

    h-index

  5. JR
    J. R. Stauffer

    California Institute of Technology, United States

    9 publications · 929 citations

    9

    h-index

1–5 of 922

Venues

  1. The Astrophysical Journal

    ApJ · 135 publications · 12K citations

    57

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    62 publications · 3.6K citations

    36

    h-index

  3. Astronomy and Astrophysics

    51 publications · 2.5K citations

    29

    h-index

  4. The Astronomical Journal

    AJ · 24 publications · 1.3K citations

    19

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 15 publications · 579 citations

    14

    h-index

1–5