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.
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2017–2026
229
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Eddington Luminosity
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C. Alcock, Edward Farhi, Angela V. Olinto · The Astrophysical Journal · 1986 · 1.2K citations
Natural Sciences, Astronomy, Physics +13
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
45 h-index
135 publications
16.1K citations

Centre National de la Recherche Scientifique
Paris, France
37 h-index
121 publications
11.3K citations
California Institute of Technology
Pasadena, United States
35 h-index
94 publications
10.2K citations
University of Cambridge
Cambridge, United Kingdom
33 h-index
109 publications
6.6K citations
Goddard Space Flight Center
Greenbelt, United States
30 h-index
82 publications
7.1K citations
University of Arizona
Tucson, United States
29 h-index
58 publications
4.8K citations
University of Southampton
Southampton, United Kingdom
28 h-index
47 publications
4.6K citations
Princeton University
Princeton, United States
28 h-index
45 publications
6K citations
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ApJ · 321 publications · 27.6K citations
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