Surface Rotation

Surface Rotation is a physical phenomenon in astrophysics denoting the rotational motion of the outer visible layer of a star, distinguished from internal or differential rotation by its observability through surface features such as sunspots or spectral line broadening.

247

Publications

14.8K

Citations

693

Authors

357

Institutions

Publications per year

2017–2026

61

Authors

693

  1. JD
    J.‐F. Donati

    Centre National de la Recherche Scientifique, France

    15 publications · 1.3K citations

    15

    h-index

  2. KG
    K. G. Strassmeier

    Leibniz Institute for Astrophysics Potsdam, Germany

    15 publications · 543 citations

    14

    h-index

  3. RA
    R. A. García

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

    13 publications · 1.4K citations

    13

    h-index

  4. AC
    A. Collier Cameron

    University of St Andrews, United Kingdom

    13 publications · 1.1K citations

    13

    h-index

  5. SM
    S. Mathur

    Centre National de la Recherche Scientifique, France

    11 publications · 1.2K citations

    11

    h-index

1–5 of 693

Venues

  1. Astronomy and Astrophysics

    62 publications · 3.7K citations

    34

    h-index

  2. 32

    h-index

  3. The Astrophysical Journal

    ApJ · 28 publications · 1.9K citations

    22

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 9 publications · 380 citations

    9

    h-index

  5. The Astrophysical Journal Letters

    4 publications · 331 citations

    4

    h-index

1–5