White Dwarf Envelopes

White Dwarf Envelopes is a theoretical construct in astrophysics that denotes the outer layers of a white dwarf star, distinguished from other stellar envelope models by its application to degenerate, Earth-sized remnants composed primarily of electron-degenerate matter and characterized by extreme surface gravities and thin non-degenerate envelopes of hydrogen or helium.

191

Publications

12K

Citations

394

Authors

199

Institutions

Publications per year

2017–2026

31

Authors

394

  1. GF
    G. Fontaine

    Université de Montréal, Canada

    11 publications · 718 citations

    11

    h-index

  2. MK
    Mariko Kato

    Keio University, Japan

    10 publications · 1.1K citations

    10

    h-index

  3. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    10 publications · 491 citations

    10

    h-index

  4. IH
    Izumi Hachisu

    The University of Tokyo, Japan

    8 publications · 1.1K citations

    8

    h-index

  5. BT
    B. T. Gänsicke

    University of Warwick, United Kingdom

    8 publications · 536 citations

    8

    h-index

1–5 of 394

Venues

  1. The Astrophysical Journal

    ApJ · 83 publications · 5.8K citations

    38

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    46 publications · 3.1K citations

    30

    h-index

  3. Astronomy and Astrophysics

    17 publications · 921 citations

    16

    h-index

  4. The Astrophysical Journal Supplement Series

    5 publications · 636 citations

    5

    h-index

  5. arXiv (Cornell University)

    Repository · 4 publications · 237 citations

    4

    h-index

1–5