White Dwarf Structure

White Dwarf Structure is a theoretical model in astrophysics that describes the internal composition and equilibrium configuration of a white dwarf star, characterized by electron degeneracy pressure supporting the star against gravitational collapse in the absence of nuclear fusion.

317

Publications

15.6K

Citations

1.2K

Authors

400

Institutions

Publications per year

2017–2026

54

Authors

1.2K

  1. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    12 publications · 489 citations

    11

    h-index

  2. DK
    D. Koester

    Christian-Albrechts-Universität zu Kiel, Germany

    10 publications · 947 citations

    10

    h-index

  3. PA
    Paul A. Bradley

    Los Alamos National Laboratory, United States

    9 publications · 526 citations

    9

    h-index

  4. MA
    M. A. Barstow

    University of Leicester, United Kingdom

    8 publications · 356 citations

    8

    h-index

  5. DE
    D. E. Winget

    The University of Texas at Austin, United States

    8 publications · 401 citations

    8

    h-index

1–5 of 1.2K

Venues

  1. The Astrophysical Journal

    ApJ · 95 publications · 5.4K citations

    43

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    61 publications · 2.2K citations

    29

    h-index

  3. Astronomy and Astrophysics

    29 publications · 1.2K citations

    18

    h-index

  4. CERN Document Server (European Organization for Nuclear Research)

    Repository · 11 publications · 435 citations

    11

    h-index

  5. Nature

    8 publications · 1.2K citations

    8

    h-index

1–5