Red Supergiants

Red Supergiants is a stellar evolutionary phase representing massive stars that have exhausted core hydrogen and expanded into luminous, cool supergiants characterized by low surface temperatures and high luminosities following hydrogen shell burning and core contraction.

840

Publications

54.1K

Citations

2K

Authors

641

Institutions

Publications per year

2017–2026

213

Variants

Red Supergiant Stars

Authors

2K

  1. GM
    G. Meynet

    University of Geneva, Switzerland

    28 publications · 5K citations

    24

    h-index

  2. PM
    Philip Massey

    Lowell Observatory, United States

    24 publications · 2.8K citations

    24

    h-index

  3. BD
    Ben Davies

    Liverpool John Moores University, United Kingdom

    33 publications · 1.8K citations

    24

    h-index

  4. BP
    B. Plez

    Université de Montpellier, France

    22 publications · 2.1K citations

    21

    h-index

  5. AC
    A. Chiavassa

    Centre National de la Recherche Scientifique, France

    26 publications · 1.3K citations

    20

    h-index

1–5 of 2K

Venues

  1. The Astrophysical Journal

    ApJ · 253 publications · 16.5K citations

    73

    h-index

  2. Astronomy and Astrophysics

    130 publications · 10.8K citations

    56

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    126 publications · 8.4K citations

    47

    h-index

  4. The Astronomical Journal

    AJ · 89 publications · 4.1K citations

    38

    h-index

  5. The Astrophysical Journal Letters

    30 publications · 1.9K citations

    25

    h-index

1–5