Eddington Limit

The Eddington Limit is a theoretical upper bound on the luminosity of a massive star, beyond which the outward radiation pressure exceeds the inward gravitational force, thereby preventing hydrostatic equilibrium and initiating intense mass loss.

932

Publications

75.5K

Citations

2.2K

Authors

680

Institutions

Publications per year

2017–2026

229

Variants

Eddington Luminosity

Authors

2.2K

  1. AC
    A. C. Fabian

    University of Cambridge, United Kingdom

    26 publications · 2.1K citations

    24

    h-index

  2. LC
    Luis C. Ho

    Peking University, China

    17 publications · 1.7K citations

    16

    h-index

  3. MV
    Marta Volonteri

    Institut d'Astrophysique de Paris, France

    14 publications · 766 citations

    14

    h-index

  4. PM
    P. Marziani

    Osservatorio Astronomico di Padova, Italy

    14 publications · 958 citations

    13

    h-index

  5. DS
    Daniel Stern

    Jet Propulsion Laboratory, United States

    12 publications · 507 citations

    12

    h-index

1–5 of 2.2K

Venues

  1. The Astrophysical Journal

    ApJ · 321 publications · 27.6K citations

    93

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    249 publications · 21.1K citations

    70

    h-index

  3. Astronomy and Astrophysics

    80 publications · 5.4K citations

    40

    h-index

  4. The Astrophysical Journal Letters

    30 publications · 1.8K citations

    25

    h-index

  5. 24

    h-index

1–5