B-type Stars

B-Type Stars is a stellar classification category within the Morgan-Keenan spectral sequence that designates hot, luminous, main-sequence stars with surface temperatures ranging from approximately 10,000 to 30,000 K and characterized by prominent neutral helium absorption lines in their ultraviolet spectra.

1.6K

Publications

88.7K

Citations

3.3K

Authors

812

Institutions

Publications per year

2017–2026

220

Authors

3.3K

  1. CA
    C. Aerts

    KU Leuven, Belgium

    45 publications · 2.1K citations

    27

    h-index

  2. DJ
    D. J. Lennon

    Instituto de Astrofísica de Canarias, Spain

    36 publications · 3K citations

    25

    h-index

  3. PL
    P. L. Dufton

    Queen's University Belfast, United Kingdom

    40 publications · 1.9K citations

    23

    h-index

  4. UH
    U. Heber

    University of Würzburg, Germany

    35 publications · 1.7K citations

    22

    h-index

  5. CN
    C. Neiner

    Centre National de la Recherche Scientifique, France

    27 publications · 1.4K citations

    20

    h-index

1–5 of 3.3K

Venues

  1. The Astrophysical Journal

    ApJ · 454 publications · 28.2K citations

    79

    h-index

  2. Astronomy and Astrophysics

    293 publications · 17.6K citations

    74

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    244 publications · 12.6K citations

    56

    h-index

  4. The Astronomical Journal

    AJ · 131 publications · 7.3K citations

    45

    h-index

  5. The Astrophysical Journal Supplement Series

    57 publications · 4.7K citations

    36

    h-index

1–5