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- W2025214347 abstract "Context.Observations of X-Ray sources harbouring a black hole and an accretion disc show the presence of at least two spectral components. One component is black-body radiation from an optically thick standard accretion disc. The other is produced in a optically thin corona and usually shows a powerlaw behaviour. Electron-proton (ep) bremsstrahlung is one of the contributing radiation mechanisms in the corona. Soft photons from the optically thick disc can Compton cool the electrons in the corona and therefore lead to a two-temperature plasma, where electrons and ions have different temperatures." @default.
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- W2025214347 date "2006-09-26" @default.
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- W2025214347 title "New electron-proton Bremsstrahlung rates for a hot plasma where the electron temperature is much smaller than the proton temperature" @default.
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