Sub-eddington Accretion

Sub-Eddington Accretion is an accretion process in which the mass inflow rate onto a compact object remains below the Eddington limit, thereby allowing stable radiative efficiency and preventing radiation pressure from halting further infall.

114

Publications

13.5K

Citations

263

Authors

207

Institutions

Publications per year

2017–2026

35

Authors

263

  1. SM
    Sera Markoff

    University of Amsterdam, Netherlands

    6 publications · 1.5K citations

    6

    h-index

  2. MM
    Matthew Middleton

    University of Southampton, United Kingdom

    6 publications · 446 citations

    6

    h-index

  3. MV
    Marta Volonteri

    Institut d'Astrophysique de Paris, France

    6 publications · 437 citations

    6

    h-index

  4. EK
    Elmar Körding

    Radboud University Nijmegen, Netherlands

    5 publications · 1.7K citations

    5

    h-index

  5. TP
    T. P. Roberts

    Durham University, United Kingdom

    5 publications · 420 citations

    5

    h-index

1–5 of 263

Venues

  1. Monthly Notices of the Royal Astronomical Society

    39 publications · 4.4K citations

    29

    h-index

  2. The Astrophysical Journal

    ApJ · 38 publications · 5.2K citations

    28

    h-index

  3. Astronomy and Astrophysics

    11 publications · 1.5K citations

    11

    h-index

  4. The Astrophysical Journal Letters

    7 publications · 806 citations

    7

    h-index

  5. 4

    h-index

1–5