White Dwarf Variability

White Dwarf Variability is a phenomenon-level concept within stellar astrophysics that denotes temporally changing photometric or spectroscopic properties intrinsic to white dwarf stars, distinguishing it from static models by characterizing their non-static structural, thermal, or magnetic behaviors.

219

Publications

9.9K

Citations

733

Authors

319

Institutions

Publications per year

2017–2026

40

Authors

733

  1. BT
    B. T. Gänsicke

    University of Warwick, United Kingdom

    18 publications · 888 citations

    16

    h-index

  2. DE
    D. E. Winget

    The University of Texas at Austin, United States

    19 publications · 906 citations

    16

    h-index

  3. TR
    T. R. Marsh

    University of Warwick, United Kingdom

    13 publications · 592 citations

    13

    h-index

  4. PS
    Paula Szkody

    University of Washington, United States

    12 publications · 561 citations

    12

    h-index

  5. JJ
    J. J. Hermes

    University of Warwick, United Kingdom

    13 publications · 464 citations

    12

    h-index

1–5 of 733

Venues

  1. The Astrophysical Journal

    ApJ · 74 publications · 3.2K citations

    34

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    68 publications · 2.6K citations

    29

    h-index

  3. Astronomy and Astrophysics

    16 publications · 637 citations

    15

    h-index

  4. The Astronomical Journal

    AJ · 7 publications · 282 citations

    7

    h-index

  5. The Astrophysical Journal Letters

    6 publications · 397 citations

    6

    h-index

1–5