Post-main-sequence Evolution

Post-Main-Sequence Evolution is a phase in stellar evolution characterized by the departure of a star from the main sequence on the Hertzsprung-Russell diagram, driven by the exhaustion of core hydrogen fusion and distinguished from earlier evolutionary stages by the initiation of shell hydrogen burning and subsequent core contraction or expansion leading to red giant or supergiant formation.

166

Publications

12.2K

Citations

433

Authors

255

Institutions

Publications per year

2017–2026

45

Authors

433

  1. DV
    Dimitri Veras

    University of Warwick, United Kingdom

    10 publications · 701 citations

    10

    h-index

  2. GM
    G. Meynet

    University of Geneva, Switzerland

    10 publications · 453 citations

    10

    h-index

  3. PE
    P. Eggenberger

    University of Geneva, Switzerland

    10 publications · 439 citations

    10

    h-index

  4. MK
    M. Kraus

    Czech Academy of Sciences, Astronomical Institute, Czechia

    6 publications · 226 citations

    6

    h-index

  5. AJ
    Alexander J. Mustill

    Lund University, Sweden

    5 publications · 312 citations

    5

    h-index

1–5 of 433

Venues

  1. The Astrophysical Journal

    ApJ · 38 publications · 2.8K citations

    25

    h-index

  2. Astronomy and Astrophysics

    34 publications · 1.6K citations

    23

    h-index

  3. 20

    h-index

  4. The Astronomical Journal

    AJ · 9 publications · 320 citations

    9

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 8 publications · 366 citations

    8

    h-index

1–5