Compact Object Accretion

Compact Object Accretion is a high-energy astrophysical process in which matter gravitationally bound to a compact object—such as a black hole, neutron star, or white dwarf—loses angular momentum and spirals inward through an accretion disk, converting gravitational potential energy into electromagnetic radiation and particle acceleration.

258

Publications

17.6K

Citations

850

Authors

371

Institutions

Publications per year

2017–2026

52

Authors

850

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    7 publications · 1.3K citations

    7

    h-index

  2. IE
    I. El Mellah

    KU Leuven, Belgium

    6 publications · 231 citations

    6

    h-index

  3. ML
    Mario Livio

    Space Telescope Science Institute, United States

    5 publications · 215 citations

    5

    h-index

  4. CP
    C. Pinto

    University of Cambridge, United Kingdom

    5 publications · 129 citations

    5

    h-index

  5. MM
    Matthew Middleton

    University of Southampton, United Kingdom

    5 publications · 144 citations

    5

    h-index

1–5 of 850

Venues

  1. The Astrophysical Journal

    ApJ · 64 publications · 5K citations

    40

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    73 publications · 5.8K citations

    37

    h-index

  3. Astronomy and Astrophysics

    37 publications · 1.7K citations

    24

    h-index

  4. Springer Link (Chiba Institute of Technology)

    Repository · 7 publications · 115 citations

    7

    h-index

  5. arXiv (Cornell University)

    Repository · 7 publications · 147 citations

    7

    h-index

1–5