Rotating Variable Stars

Rotating Variable Stars is a class of variable stars whose observed brightness variations are primarily caused by the rotational modulation of surface features such as starspots, ellipsoidal deformations, or brightness inhomogeneities, distinguishing them from pulsating or eclipsing variable stars.

75

Publications

5K

Citations

284

Authors

132

Institutions

Publications per year

2017–2026

8

Variants

Rotational Variables

Authors

284

  1. RJ
    Rahul Jayaraman

    Massachusetts Institute of Technology, United States

    2 publications · 38 citations

    2

    h-index

  2. MD
    M.-A. Dupret

    University of Liège, Belgium

    2 publications · 58 citations

    2

    h-index

  3. JM
    J. Montalbán

    University of Liège, Belgium

    2 publications · 67 citations

    2

    h-index

  4. CH
    Cecilia Helena Payne Gaposchkin

    2 publications · 92 citations

    2

    h-index

  5. GH
    G. Handler

    University of Vienna, Austria

    2 publications · 31 citations

    2

    h-index

1–5 of 284

Venues

  1. The Astrophysical Journal

    ApJ · 22 publications · 1K citations

    17

    h-index

  2. 10

    h-index

  3. The Astronomical Journal

    AJ · 11 publications · 502 citations

    10

    h-index

  4. Communications in Asteroseismology

    CoAst · 6 publications · 167 citations

    6

    h-index

  5. Astronomy and Astrophysics

    5 publications · 230 citations

    5

    h-index

1–5