Spectroscopic Variability

Spectroscopic Variability is a systematic change in the spectral characteristics of a star, such as line intensity, shape, or Doppler shift, arising from intrinsic stellar processes or binary orbital motion, as opposed to variations in total electromagnetic flux.

489

Publications

20.4K

Citations

1.9K

Authors

642

Institutions

Publications per year

2017–2026

77

Authors

1.9K

  1. CA
    C. Aerts

    KU Leuven, Belgium

    17 publications · 786 citations

    16

    h-index

  2. RA
    Ronald A. Schorn

    Jet Propulsion Laboratory, United States

    11 publications · 250 citations

    10

    h-index

  3. CN
    C. Neiner

    Centre National de la Recherche Scientifique, France

    9 publications · 339 citations

    9

    h-index

  4. GR
    G. Rauw

    University of Liège, Belgium

    7 publications · 219 citations

    7

    h-index

  5. KL
    K. Lefever

    KU Leuven, Belgium

    7 publications · 443 citations

    7

    h-index

1–5 of 1.9K

Venues

  1. The Astrophysical Journal

    ApJ · 109 publications · 5.2K citations

    43

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    79 publications · 3.2K citations

    32

    h-index

  3. Astronomy and Astrophysics

    85 publications · 3.1K citations

    31

    h-index

  4. The Astronomical Journal

    AJ · 41 publications · 1.7K citations

    25

    h-index

  5. Icarus

    16 publications · 563 citations

    14

    h-index

1–5