Late-stage Stellar Evolution

Late-Stage Stellar Evolution is a theoretical framework in astrophysics that describes the final phases of a star's lifecycle, distinguished from earlier evolutionary stages by the exhaustion of core nuclear fuel and the onset of advanced burning processes, mass loss, and structural instabilities leading to supernova progenitor states.

102

Publications

7.2K

Citations

262

Authors

161

Institutions

Publications per year

2017–2026

8

Authors

262

  1. AM
    A. Maeder

    Global Social Observatory, Switzerland

    8 publications · 2.3K citations

    8

    h-index

  2. GM
    G. Meynet

    University of Geneva, Switzerland

    7 publications · 2.3K citations

    7

    h-index

  3. RH
    Raphaël Hirschi

    Keele University, United Kingdom

    5 publications · 732 citations

    5

    h-index

  4. CH
    Chûshirô Hayashi

    Kyoto University, Japan

    4 publications · 210 citations

    4

    h-index

  5. QA
    Q. A. Parker

    Australian Astronomical Observatory, Australia

    3 publications · 129 citations

    3

    h-index

1–5 of 262

Venues

  1. Astronomy and Astrophysics

    18 publications · 2.5K citations

    16

    h-index

  2. The Astrophysical Journal

    ApJ · 19 publications · 1.3K citations

    15

    h-index

  3. 11

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 283 citations

    4

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 4 publications · 131 citations

    4

    h-index

1–5