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- W1611065350 abstract "We use a new code to simulate the radiation and kinetic processes in the X‐ray emitting region around accreting black holes and constrain the magnetic field and temperature of the hot protons in the corona of Cygnus X‐1. In the hard state we find a magnetic field below equipartition with radiation, suggesting that the corona is not powered through magnetic field dissipation (as assumed in most accretion disc corona models). On the other hand, our results also point toward proton temperatures that are substantially lower than typical temperatures of the ADAF models. Finally, we show that in both spectral states Comptonising plasma could be powered essentially through power‐law acceleration of non‐thermal electrons, which are then partly thermalised by the synchrotron and Coulomb boiler. This suggests that, contrary to current beliefs, the corona of the HSS and that of the LHS could be of very similar nature. The differences between the LHS and HSS coronal spectra would then be predominantly caused by the strong disc soft cooling emission which is present in the HSS and absent in the LHS." @default.
- W1611065350 created "2016-06-24" @default.
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- W1611065350 date "2009-01-01" @default.
- W1611065350 modified "2023-09-25" @default.
- W1611065350 title "Synchrotron and Coulomb Boiler in Cygnus X-1" @default.
- W1611065350 doi "https://doi.org/10.1063/1.3149409" @default.
- W1611065350 hasPublicationYear "2009" @default.
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