Accretion Disk Variability

Accretion Disk Variability is a physical phenomenon characterized by temporal fluctuations in the radiative output of an accretion disk, arising from dynamic processes such as viscosity changes, instabilities, or perturbations in the accreting plasma under the influence of strong gravitational fields.

118

Publications

6.3K

Citations

354

Authors

274

Institutions

Publications per year

2017–2026

30

Authors

354

  1. VK
    V. Karas

    Czech Academy of Sciences, Astronomical Institute, Czechia

    4 publications · 78 citations

    4

    h-index

  2. ME
    Michael Eracleous

    Pennsylvania State University, United States

    4 publications · 175 citations

    4

    h-index

  3. SS
    Simone Scaringi

    University of Southampton, United Kingdom

    3 publications · 99 citations

    3

    h-index

  4. BC
    B. Czerny

    Nicolaus Copernicus Astronomical Center, Poland

    3 publications · 109 citations

    3

    h-index

  5. SM
    Shin Mineshige

    Kyoto University, Japan

    3 publications · 873 citations

    3

    h-index

1–5 of 354

Venues

  1. The Astrophysical Journal

    ApJ · 42 publications · 2.2K citations

    25

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.2K citations

    18

    h-index

  3. Astronomy and Astrophysics

    14 publications · 504 citations

    13

    h-index

  4. arXiv (Cornell University)

    Repository · 4 publications · 64 citations

    4

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 4 publications · 400 citations

    4

    h-index

1–5