Oosterhoff Classification

Oosterhoff Classification is a taxonomic framework in stellar astronomy that distinguishes globular clusters based on the observed period distribution of their RR Lyrae variable stars, specifically categorizing them into two distinct groups according to the average pulsation periods of these stars.

114

Publications

5.1K

Citations

268

Authors

152

Institutions

Publications per year

2017–2026

11

Authors

268

  1. MC
    M. Catelan

    Pontificia Universidad Católica de Chile, Chile

    20 publications · 827 citations

    16

    h-index

  2. GC
    G. Clementini

    Astronomical Observatory of Capodimonte, Italy

    13 publications · 597 citations

    13

    h-index

  3. BJ
    B. J. Pritzl

    Michigan State University, United States

    10 publications · 471 citations

    10

    h-index

  4. MM
    M. Marconi

    Astronomical Observatory of Capodimonte, Italy

    10 publications · 505 citations

    10

    h-index

  5. VR
    V. Ripepi

    Astronomical Observatory of Capodimonte, Italy

    9 publications · 470 citations

    9

    h-index

1–5 of 268

Venues

  1. The Astrophysical Journal

    ApJ · 36 publications · 1.8K citations

    25

    h-index

  2. The Astronomical Journal

    AJ · 37 publications · 2K citations

    24

    h-index

  3. 11

    h-index

  4. Publications of the Astronomical Society of the Pacific

    PASP · 3 publications · 120 citations

    3

    h-index

  5. The Astrophysical Journal Supplement Series

    3 publications · 146 citations

    3

    h-index

1–5