Main Sequence Evolution

Main Sequence Evolution is a theoretical framework in stellar astrophysics that describes the phase of a star's life during which it fuses hydrogen into helium in its core, maintaining a stable structure determined by the balance between gravitational contraction and radiative pressure, thereby defining the dominant trajectory of stars on the Hertzsprung-Russell diagram.

779

Publications

71K

Citations

1.7K

Authors

593

Institutions

Publications per year

2017–2026

111

Authors

1.7K

  1. GM
    G. Meynet

    University of Geneva, Switzerland

    12 publications · 2.8K citations

    12

    h-index

  2. NL
    N. Langer

    University of Bonn, Germany

    11 publications · 3.5K citations

    11

    h-index

  3. AM
    A. Maeder

    Global Social Observatory, Switzerland

    10 publications · 2.9K citations

    10

    h-index

  4. JI
    Jr. Iben Icko

    University of Illinois System, United States

    10 publications · 1.3K citations

    10

    h-index

  5. PD
    P. Demarque

    Yale University, United States

    10 publications · 469 citations

    10

    h-index

1–5 of 1.7K

Venues

  1. The Astrophysical Journal

    ApJ · 274 publications · 29.6K citations

    78

    h-index

  2. Astronomy and Astrophysics

    118 publications · 12.3K citations

    52

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    126 publications · 10.5K citations

    48

    h-index

  4. The Astronomical Journal

    AJ · 43 publications · 2K citations

    25

    h-index

  5. The Astrophysical Journal Supplement Series

    18 publications · 3.8K citations

    16

    h-index

1–5