Massive Stars

Massive Stars is a class of stars characterized by having initial masses exceeding approximately eight solar masses, distinguished from lower-mass stars by their dominant evolution pathways, higher luminosities, and ultimate fates as supernovae or compact remnants.

13.1K

Publications

1M

Citations

22.4K

Authors

2.5K

Institutions

Publications per year

2017–2026

3.2K

Authors

22.4K

  1. NL
    N. Langer

    University of Bonn, Germany

    195 publications · 28.7K citations

    79

    h-index

  2. AD
    A. de Koter

    University of Amsterdam, Netherlands

    114 publications · 14.1K citations

    60

    h-index

  3. JS
    J. S. Vink

    Armagh Observatory & Planetarium, United Kingdom

    137 publications · 13K citations

    60

    h-index

  4. GM
    G. Meynet

    University of Geneva, Switzerland

    119 publications · 13.7K citations

    59

    h-index

  5. SE
    S. E. de Mink

    University of Amsterdam, Netherlands

    99 publications · 12.6K citations

    57

    h-index

1–5 of 22.4K

Venues

  1. The Astrophysical Journal

    ApJ · 3.7K publications · 339.4K citations

    251

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    2.5K publications · 176.6K citations

    182

    h-index

  3. Astronomy and Astrophysics

    2K publications · 140.3K citations

    161

    h-index

  4. The Astronomical Journal

    AJ · 591 publications · 35.2K citations

    90

    h-index

  5. The Astrophysical Journal Letters

    385 publications · 24K citations

    82

    h-index

1–5