Massive Star Evolution

Massive Star Evolution is a theoretical astrophysical framework that models the lifecycle stages of stars with initial masses greater than approximately eight solar masses, distinguishing itself by incorporating nuclear burning phases, mass loss mechanisms, and internal structure changes leading to supernova progenitors.

1.4K

Publications

132.2K

Citations

3.1K

Authors

868

Institutions

Publications per year

2017–2026

358

Authors

3.1K

  1. NL
    N. Langer

    University of Bonn, Germany

    57 publications · 10.3K citations

    42

    h-index

  2. JS
    J. S. Vink

    Armagh Observatory & Planetarium, United Kingdom

    51 publications · 4.3K citations

    38

    h-index

  3. HS
    H. Sana

    KU Leuven, Belgium

    43 publications · 4.2K citations

    34

    h-index

  4. GM
    G. Meynet

    University of Geneva, Switzerland

    47 publications · 4.7K citations

    32

    h-index

  5. AD
    A. de Koter

    University of Amsterdam, Netherlands

    34 publications · 3.4K citations

    29

    h-index

1–5 of 3.1K

Venues

  1. The Astrophysical Journal

    ApJ · 414 publications · 40.5K citations

    105

    h-index

  2. Astronomy and Astrophysics

    262 publications · 20.7K citations

    77

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    238 publications · 18.1K citations

    73

    h-index

  4. The Astronomical Journal

    AJ · 48 publications · 3.2K citations

    30

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 46 publications · 2.4K citations

    30

    h-index

1–5