Stellar Evolutionary Models

Stellar Evolutionary Models is a theoretical framework that describes the physical processes and structural changes governing the life cycle of stars from their formation in molecular clouds through the main sequence, with particular emphasis on pre-main-sequence contraction, accretion, and energy transport mechanisms distinguishing it from post-main-sequence evolutionary theories.

2.7K

Publications

256.6K

Citations

4.6K

Authors

1K

Institutions

Publications per year

2017–2026

455

Variants

Stellar Evolution Models

Authors

4.6K

  1. GM
    G. Meynet

    University of Geneva, Switzerland

    66 publications · 9K citations

    41

    h-index

  2. SC
    S. Cassisi

    Collurania Teramo Observatory, Italy

    38 publications · 5.9K citations

    30

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    43 publications · 5.2K citations

    29

    h-index

  4. LG
    L. Girardi

    Osservatorio Astronomico di Padova, Italy

    33 publications · 13.6K citations

    29

    h-index

  5. AM
    A. Maeder

    Global Social Observatory, Switzerland

    39 publications · 6.6K citations

    29

    h-index

1–5 of 4.6K

Venues

  1. The Astrophysical Journal

    ApJ · 916 publications · 90.4K citations

    142

    h-index

  2. Astronomy and Astrophysics

    493 publications · 39.7K citations

    93

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    406 publications · 48.1K citations

    90

    h-index

  4. The Astrophysical Journal Supplement Series

    73 publications · 19.1K citations

    54

    h-index

  5. The Astronomical Journal

    AJ · 99 publications · 5.6K citations

    44

    h-index

1–5