Radial Velocity Variability

Radial Velocity Variability is the systematic variation in the line-of-sight component of a star's motion relative to an observer, as measured through Doppler shifts in spectral lines, that arises from intrinsic astrophysical processes such as rotational modulation, pulsations, accretion dynamics, or the presence of unseen companions during the pre-main sequence evolutionary phase.

825

Publications

46.5K

Citations

2.6K

Authors

691

Institutions

Publications per year

2017–2026

142

Authors

2.6K

  1. SU
    S. Udry

    University of Geneva, Switzerland

    54 publications · 4.9K citations

    37

    h-index

  2. MM
    M. Mayor

    University of Geneva, Switzerland

    39 publications · 3.7K citations

    30

    h-index

  3. FP
    F. Pepe

    University of Geneva, Switzerland

    37 publications · 3.8K citations

    28

    h-index

  4. AP
    A. P. Hatzes

    Thüringer Landessternwarte Tautenburg, Germany

    38 publications · 2.8K citations

    28

    h-index

  5. DQ
    D. Queloz

    University of Geneva, Switzerland

    27 publications · 3.5K citations

    24

    h-index

1–5 of 2.6K

Venues

  1. The Astrophysical Journal

    ApJ · 201 publications · 13.4K citations

    62

    h-index

  2. Astronomy and Astrophysics

    155 publications · 9.9K citations

    53

    h-index

  3. 45

    h-index

  4. The Astronomical Journal

    AJ · 72 publications · 3.2K citations

    35

    h-index

  5. arXiv (Cornell University)

    Repository · 22 publications · 757 citations

    17

    h-index

1–5