Hot Accretion Flows

Hot Accretion Flows is a theoretical model of radiatively inefficient accretion onto compact objects characterized by a geometrically thick, optically thin plasma flow with a sub-Keplerian rotation profile and a temperature close to the virial temperature of the gravitational potential.

203

Publications

15K

Citations

351

Authors

247

Institutions

Publications per year

2017–2026

51

Variants

Riafs

Authors

351

  1. DB
    De-Fu Bu

    Shanghai Astronomical Observatory, China

    13 publications · 1K citations

    12

    h-index

  2. FX
    Fu‐Guo Xie

    Shanghai Astronomical Observatory, China

    11 publications · 533 citations

    11

    h-index

  3. RN
    Ramesh Narayan

    Center for Astrophysics Harvard & Smithsonian, United States

    11 publications · 4K citations

    11

    h-index

  4. AA
    A. A. Zdziarski

    Nicolaus Copernicus Astronomical Center, Poland

    11 publications · 867 citations

    11

    h-index

  5. SA
    Shahram Abbassi

    Ferdowsi University of Mashhad, Iran

    9 publications · 176 citations

    9

    h-index

1–5 of 351

Venues

  1. The Astrophysical Journal

    ApJ · 67 publications · 6K citations

    39

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    65 publications · 3.6K citations

    30

    h-index

  3. Astronomy and Astrophysics

    14 publications · 445 citations

    13

    h-index

  4. The Astrophysical Journal Letters

    7 publications · 388 citations

    7

    h-index

  5. 3

    h-index

1–5