Correlating spectral and timing properties in the evolving jet of the micro blazar MAXI J1836-194
M. Lucchini,
T. D. Russell,
S. B. Markoff
et al.
Abstract:During outbursts, the observational properties of black hole X-ray binaries (BHXBs) vary on timescales of days to months. These relatively short timescales make these systems ideal laboratories to probe the coupling between accreting material and outflowing jets as a the accretion rate varies. In particular, the origin of the hard X-ray emission is poorly understood and highly debated. This spectral component, which has a power-law shape, is due to Comptonisation of photons near the black hole, but it is uncle… Show more
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