Blue Supergiants

Blue Supergiants is a stellar classification denoting a massive, luminous star in the late evolutionary phase characterized by high surface temperatures and spectral types O or B, distinguished from other supergiants by its prominent blue color and position on the upper left portion of the Hertzsprung-Russell diagram.

328

Publications

18.2K

Citations

718

Authors

375

Institutions

Publications per year

2017–2026

66

Variants

Blue Supergiant

Authors

718

  1. RK
    Rolf‐Peter Kudritzki

    University of Hawaii System, United States

    12 publications · 642 citations

    12

    h-index

  2. MA
    Miguel A. Urbaneja

    University of Hawaii System, United States

    10 publications · 514 citations

    10

    h-index

  3. NL
    N. Langer

    University of Bonn, Germany

    10 publications · 825 citations

    10

    h-index

  4. FB
    Fabio Bresolin

    University of Hawaii System, United States

    9 publications · 519 citations

    9

    h-index

  5. RM
    R. M. Humphreys

    University of Minnesota, United States

    9 publications · 994 citations

    9

    h-index

1–5 of 718

Venues

  1. The Astrophysical Journal

    ApJ · 88 publications · 6.1K citations

    40

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    48 publications · 2.5K citations

    28

    h-index

  3. Astronomy and Astrophysics

    44 publications · 2.1K citations

    28

    h-index

  4. The Astronomical Journal

    AJ · 40 publications · 1.7K citations

    26

    h-index

  5. Springer Link (Chiba Institute of Technology)

    Repository · 10 publications · 418 citations

    10

    h-index

1–5