The Eddington Limit is the maximum luminosity a star or an accreting black hole can achieve when the outward pressure of radiation balances the inward pull of gravity. This limit is crucial in understanding how massive objects, such as black holes and active galactic nuclei, can grow and evolve. When a system exceeds this limit, radiation pressure can blow away the surrounding material, affecting accretion processes and the characteristics of active galactic nuclei.
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