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- W2053539462 abstract "The galactic black hole binary systems give an observational template showing how the accretion flow changes as a function of increasing mass accretion rate, or L/L Edd. These data can be synthesised with theoretical models of the accretion flow to give a coherent picture of accretion in strong gravity, in which the major hard-soft spectral transition is triggered by a change in the nature and geometry of the inner accretion flow from a hot, optically thin plasma to a cool, optically thick accretion disc. However, a straightforward application of these models to AGN gives clear discrepancies in overall spectral shape. Either the underlying accretion model is wrong, despite its success in describing the Galactic systems and/or there is additional physics which breaks the simple scaling from stellar to supermassive black holes.Keywordsblack holesaccretion flows" @default.
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- W2053539462 date "2007-01-26" @default.
- W2053539462 modified "2023-09-25" @default.
- W2053539462 title "Accretion in strong gravity: From galactic to supermassive black holes" @default.
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- W2053539462 doi "https://doi.org/10.1007/1-4020-4085-7_20" @default.
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