Eddington Limit

Some articles on eddington, eddington limit:

Eddington Luminosity
... The Eddington luminosity (also referred to as the Eddington limit) of a source is defined as the maximum luminosity where the continuum radiation force outwards balances the gravitational ... When exceeding the Eddington luminosity, a star would initiate a very intense continuum-driven stellar wind from its outer layers ... massive stars have luminosities far below the Eddington luminosity, however, their winds are mostly driven by the less intense line absorption ...
Hypergiant - Stability
... increases greatly with mass, the luminosity of hypergiants often lies very close to the Eddington limit, which is the luminosity at which the force of ... Above the Eddington limit, the star would generate so much radiation that parts of its outer layers would be thrown off in massive outbursts this would ... that Eta Carinae may occasionally exceed the Eddington limit ...
Eddington Luminosity - Super-Eddington Luminosities
... The role of the Eddington limit in today’s research lies in explaining the very high mass loss rates seen in for example the series of outbursts of η Carinae in 1840–1860 ... This can be done with the help of the super-Eddington continuum driven winds ... Gamma-ray bursts, novae and supernovae are examples of systems exceeding their Eddington luminosity by a large factor for very short times, resulting in short and highly intensive mass ...

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