Horizontal Branch Morphology

Horizontal Branch Morphology is a stellar population diagnostic metric that characterizes the distribution and evolutionary phases of low-mass stars along the horizontal branch in globular clusters, distinguished by its sensitivity to age, metallicity, and helium abundance variations.

582

Publications

40.6K

Citations

1K

Authors

447

Institutions

Publications per year

2017–2026

46

Authors

1K

  1. GP
    G. Piotto

    Osservatorio Astronomico di Padova, Italy

    28 publications · 3.2K citations

    26

    h-index

  2. SC
    S. Cassisi

    Collurania Teramo Observatory, Italy

    26 publications · 1.9K citations

    22

    h-index

  3. FR
    F. R. Ferraro

    Osservatorio astronomico di Bologna, Italy

    20 publications · 1.5K citations

    20

    h-index

  4. FD
    F. D’Antona

    Astronomical Observatory of Rome, Italy

    19 publications · 1.8K citations

    19

    h-index

  5. SO
    S. Ortolani

    University of Padua, Italy

    23 publications · 1.5K citations

    18

    h-index

1–5 of 1K

Venues

  1. The Astrophysical Journal

    ApJ · 164 publications · 10.2K citations

    55

    h-index

  2. The Astronomical Journal

    AJ · 116 publications · 10.6K citations

    45

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    89 publications · 7.3K citations

    38

    h-index

  4. Astronomy and Astrophysics

    54 publications · 3.3K citations

    33

    h-index

  5. The Astrophysical Journal Letters

    17 publications · 809 citations

    14

    h-index

1–5