Accretion Onto Compact Objects

Accretion Onto Compact Objects is a theoretical framework in astrophysics that describes the dynamical and radiative processes by which matter gravitationally bound to a compact object—such as a black hole, neutron star, or white dwarf—loses angular momentum and energy to spiral inward and accumulate onto the object’s surface or event horizon, distinguishing it from general accretion phenomena by the dominance of extreme gravitational fields, relativistic effects, and high-energy emission mechanisms.

491

Publications

40K

Citations

1.3K

Authors

556

Institutions

Publications per year

2017–2026

136

Authors

1.3K

  1. CB
    Cosimo Bambi

    Fudan University, China

    9 publications · 418 citations

    9

    h-index

  2. ZS
    Zdeněk Stuchlík

    Silesian University in Opava, Czechia

    8 publications · 477 citations

    8

    h-index

  3. AE
    Avery E. Broderick

    Perimeter Institute, Canada

    7 publications · 954 citations

    7

    h-index

  4. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    7 publications · 1.6K citations

    7

    h-index

  5. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    7 publications · 2.8K citations

    7

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 135 publications · 11.4K citations

    56

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    92 publications · 8.1K citations

    40

    h-index

  3. Astronomy and Astrophysics

    35 publications · 1.7K citations

    23

    h-index

  4. Classical and Quantum Gravity

    16 publications · 1.4K citations

    16

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 17 publications · 751 citations

    16

    h-index

1–5