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Going with the flow: can the base of jets subsume the role of compact accretion disk coronae?

ASTROPHYSICAL JOURNAL, no. 2 (2005): 1203-1216

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The hard state of X-ray binaries (XRBs) is characterized by a power-law spectrum in the X-ray band and a flat/inverted radio/IR spectrum associated with occasionally imaged compact jets. It has generally been thought that the hard X-rays result from Compton upscattering of thermal accretion disk photons by a hot, coronal plasma whose prop...更多

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