White Dwarfs

White Dwarf is a stellar remnant constituting the final evolutionary state of low- to intermediate-mass stars, distinguished by its high density, electron-degenerate core, and lack of active nuclear fusion.

7.9K

Publications

507K

Citations

11.7K

Authors

1.9K

Institutions

Publications per year

2017–2026

1.7K

Authors

11.7K

  1. BT
    B. T. Gänsicke

    University of Warwick, United Kingdom

    285 publications · 17.5K citations

    72

    h-index

  2. DK
    D. Koester

    Christian-Albrechts-Universität zu Kiel, Germany

    189 publications · 12.4K citations

    61

    h-index

  3. TR
    T. R. Marsh

    University of Warwick, United Kingdom

    168 publications · 14.8K citations

    57

    h-index

  4. PB
    P. Bergeron

    Université de Montréal, Canada

    131 publications · 11.6K citations

    55

    h-index

  5. JL
    James Liebert

    University of Arizona, United States

    119 publications · 9K citations

    50

    h-index

1–5 of 11.7K

Venues

  1. The Astrophysical Journal

    ApJ · 2.6K publications · 192.7K citations

    177

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    1.7K publications · 86.5K citations

    122

    h-index

  3. Astronomy and Astrophysics

    746 publications · 38.9K citations

    94

    h-index

  4. The Astronomical Journal

    AJ · 349 publications · 17.6K citations

    67

    h-index

  5. The Astrophysical Journal Supplement Series

    125 publications · 31.3K citations

    65

    h-index

1–5