Main-sequence Stars

Main-Sequence Stars is a class of stars in stellar astrophysics that are in the long-lived, hydrostatic-equilibrium phase of their evolution during which they generate energy primarily by fusing hydrogen into helium in their cores and consequently occupy the main sequence locus in the Hertzsprung–Russell diagram.

2.6K

Publications

189K

Citations

4.5K

Authors

1K

Institutions

Publications per year

2017–2026

371

Authors

4.5K

  1. NL
    N. Langer

    University of Bonn, Germany

    29 publications · 3.2K citations

    22

    h-index

  2. HS
    Hideyuki Saio

    Tohoku University, Japan

    23 publications · 1.8K citations

    19

    h-index

  3. DL
    David L. Lambert

    The University of Texas at Austin, United States

    20 publications · 1.6K citations

    19

    h-index

  4. JD
    J. D. Landstreet

    Western University, Canada

    21 publications · 1.8K citations

    19

    h-index

  5. GM
    G. Michaud

    Université de Montréal, Canada

    22 publications · 1.4K citations

    18

    h-index

1–5 of 4.5K

Venues

  1. The Astrophysical Journal

    ApJ · 795 publications · 72.5K citations

    125

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    428 publications · 25.9K citations

    84

    h-index

  3. Astronomy and Astrophysics

    326 publications · 20.3K citations

    76

    h-index

  4. The Astronomical Journal

    AJ · 224 publications · 12.3K citations

    62

    h-index

  5. The Astrophysical Journal Supplement Series

    58 publications · 13.4K citations

    39

    h-index

1–5