Rr Lyrae Variables

RR Lyrae Variables is a class of pulsating variable stars that belong to the category of horizontal branch stars in globular clusters, distinguished by their characteristic light curves, periods typically between 0.2 and 1 day, and use as standard candles for measuring cosmic distances.

849

Publications

59K

Citations

2.5K

Authors

603

Institutions

Publications per year

2017–2026

150

Authors

2.5K

  1. MM
    M. Marconi

    Astronomical Observatory of Capodimonte, Italy

    48 publications · 12K citations

    30

    h-index

  2. GC
    G. Clementini

    Astronomical Observatory of Capodimonte, Italy

    39 publications · 11.6K citations

    30

    h-index

  3. GB
    G. Bono

    Astronomical Observatory of Rome, Italy

    43 publications · 2.3K citations

    27

    h-index

  4. MC
    M. Catelan

    Pontificia Universidad Católica de Chile, Chile

    38 publications · 2.5K citations

    27

    h-index

  5. AR
    A. R. Walker

    Cerro Tololo Inter-American Observatory, Chile

    33 publications · 1.7K citations

    24

    h-index

1–5 of 2.5K

Venues

  1. The Astrophysical Journal

    ApJ · 212 publications · 12.4K citations

    62

    h-index

  2. The Astronomical Journal

    AJ · 196 publications · 10.4K citations

    61

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    157 publications · 6.6K citations

    42

    h-index

  4. Astronomy and Astrophysics

    75 publications · 17.1K citations

    39

    h-index

  5. The Astrophysical Journal Supplement Series

    30 publications · 4.2K citations

    23

    h-index

1–5