O-type Stars

O-Type Stars is a stellar classification category within the framework of stellar astrophysics denoting massive, hot stars of spectral type O, distinguished by their dominant ionized helium absorption lines and prominent ultraviolet continua indicative of high effective temperatures and strong stellar winds.

1.2K

Publications

85.9K

Citations

2.3K

Authors

685

Institutions

Publications per year

2017–2026

166

Variants

O-class Stars

Authors

2.3K

  1. NR
    N. R. Walborn

    Space Telescope Science Institute, United States

    77 publications · 7.4K citations

    45

    h-index

  2. HS
    H. Sana

    KU Leuven, Belgium

    59 publications · 4.9K citations

    40

    h-index

  3. CJ
    C. J. Evans

    UK Astronomy Technology Centre, United Kingdom

    61 publications · 5.8K citations

    40

    h-index

  4. AD
    A. de Koter

    University of Amsterdam, Netherlands

    48 publications · 5.5K citations

    37

    h-index

  5. JM
    J. Maíz Apellániz

    Instituto de Astrofísica de Andalucía, Spain

    50 publications · 5K citations

    36

    h-index

1–5 of 2.3K

Venues

  1. The Astrophysical Journal

    ApJ · 403 publications · 27.4K citations

    84

    h-index

  2. Astronomy and Astrophysics

    246 publications · 18.5K citations

    69

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    166 publications · 10.3K citations

    53

    h-index

  4. The Astronomical Journal

    AJ · 85 publications · 5.3K citations

    42

    h-index

  5. The Astrophysical Journal Supplement Series

    39 publications · 7.9K citations

    30

    h-index

1–5