White Dwarf Core Composition

White Dwarf Core Composition is a scientific construct that specifies the elemental and isotopic makeup of the dense, degenerate interior region of a white dwarf star, distinguishing it from atmospheric and envelope compositions by reflecting the remnant nuclear burning products and subsequent gravitational settling processes of stellar evolution.

107

Publications

5.9K

Citations

189

Authors

137

Institutions

Publications per year

2017–2026

27

Authors

189

  1. LG
    L. G. Althaus

    Universidad Nacional de La Plata, Argentina

    7 publications · 216 citations

    7

    h-index

  2. GF
    G. Fontaine

    Université de Montréal, Canada

    7 publications · 388 citations

    7

    h-index

  3. PB
    P. Brassard

    Université de Montréal, Canada

    6 publications · 479 citations

    6

    h-index

  4. AB
    Amy Bonsor

    University of Cambridge, United Kingdom

    6 publications · 268 citations

    6

    h-index

  5. DK
    D. Koester

    Christian-Albrechts-Universität zu Kiel, Germany

    5 publications · 168 citations

    6

    h-index

1–5 of 189

Venues

  1. The Astrophysical Journal

    ApJ · 40 publications · 2.7K citations

    27

    h-index

  2. 12

    h-index

  3. Astronomy and Astrophysics

    10 publications · 373 citations

    10

    h-index

  4. The Astrophysical Journal Letters

    6 publications · 247 citations

    6

    h-index

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

    Repository · 4 publications · 166 citations

    4

    h-index

1–5