Db White Dwarfs

DB White Dwarfs is a subclass of white dwarf stars characterized by a helium-dominated atmosphere with no detectable hydrogen, distinguished spectroscopically by the presence of neutral helium absorption lines in its optical spectrum.

207

Publications

11.6K

Citations

446

Authors

227

Institutions

Publications per year

2017–2026

30

Authors

446

  1. PB
    P. Bergeron

    Université de Montréal, Canada

    18 publications · 1.9K citations

    17

    h-index

  2. DE
    D. E. Winget

    The University of Texas at Austin, United States

    18 publications · 1.2K citations

    15

    h-index

  3. DK
    D. Koester

    Christian-Albrechts-Universität zu Kiel, Germany

    15 publications · 1.1K citations

    12

    h-index

  4. HL
    H. L. Shipman

    University of Delaware, United States

    11 publications · 383 citations

    11

    h-index

  5. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    10 publications · 853 citations

    10

    h-index

1–5 of 446

Venues

  1. The Astrophysical Journal

    ApJ · 88 publications · 5.1K citations

    40

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    38 publications · 1.5K citations

    22

    h-index

  3. Astronomy and Astrophysics

    25 publications · 1.5K citations

    19

    h-index

  4. The Astronomical Journal

    AJ · 16 publications · 616 citations

    14

    h-index

  5. The Astrophysical Journal Supplement Series

    10 publications · 1.2K citations

    10

    h-index

1–5