White Dwarf Evolution

White Dwarf Evolution is a theoretical framework within stellar astrophysics that describes the cooling and structural changes of white dwarfs over time as they radiate away residual thermal energy in the absence of nuclear fusion.

984

Publications

62.7K

Citations

1.5K

Authors

578

Institutions

Publications per year

2017–2026

208

Authors

1.5K

  1. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    76 publications · 4.4K citations

    35

    h-index

  2. BT
    B. T. Gänsicke

    University of Warwick, United Kingdom

    51 publications · 3.8K citations

    34

    h-index

  3. JI
    J. Isern

    Institut d'Estudis Espacials de Catalunya, Spain

    44 publications · 3.4K citations

    32

    h-index

  4. EG
    E. Garcı́a–Berro

    Universitat Politècnica de Catalunya, Spain

    43 publications · 3.4K citations

    31

    h-index

  5. MR
    M. R. Schreiber

    University of Valparaíso, Chile

    35 publications · 2.2K citations

    27

    h-index

1–5 of 1.5K

Venues

  1. The Astrophysical Journal

    ApJ · 324 publications · 25.6K citations

    83

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    222 publications · 11.8K citations

    61

    h-index

  3. Astronomy and Astrophysics

    120 publications · 7.7K citations

    46

    h-index

  4. The Astrophysical Journal Letters

    23 publications · 1K citations

    22

    h-index

  5. The Astronomical Journal

    AJ · 16 publications · 562 citations

    14

    h-index

1–5