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Eddington limit

/ˈɛdɪŋtən/
noun
1.
(astronomy) the theoretical upper limit of luminosity that a star of a given mass can reach; occurs when the outward force of the radiation just balances the inward gravitational force
Word Origin
C20: named after A. S. Eddington (1882–1944), English astronomer and physicist
Collins English Dictionary - Complete & Unabridged 2012 Digital Edition
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