Horizontal Branch Evolution

Horizontal Branch Evolution is a phase in stellar evolution characterized by the stable helium core burning and hydrogen shell burning in low- to intermediate-mass stars after they ascend the red giant branch and settle on the horizontal branch in the Hertzsprung–Russell diagram.

355

Publications

26K

Citations

709

Authors

357

Institutions

Publications per year

2017–2026

32

Authors

709

  1. SC
    S. Cassisi

    Collurania Teramo Observatory, Italy

    27 publications · 2.7K citations

    25

    h-index

  2. VC
    V. Castellani

    University of Pisa, Italy

    19 publications · 955 citations

    17

    h-index

  3. MS
    M. Salaris

    Liverpool John Moores University, United Kingdom

    16 publications · 1.4K citations

    16

    h-index

  4. AV
    A. V. Sweigart

    Goddard Space Flight Center, United States

    15 publications · 1.2K citations

    14

    h-index

  5. GP
    G. Piotto

    Osservatorio Astronomico di Padova, Italy

    14 publications · 1.6K citations

    14

    h-index

1–5 of 709

Venues

  1. The Astrophysical Journal

    ApJ · 102 publications · 7.6K citations

    48

    h-index

  2. Astronomy and Astrophysics

    52 publications · 3.1K citations

    34

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    49 publications · 4.4K citations

    28

    h-index

  4. The Astronomical Journal

    AJ · 46 publications · 3.1K citations

    27

    h-index

  5. The Astrophysical Journal Letters

    15 publications · 603 citations

    13

    h-index

1–5