Time dependent accretion onto a black hole in a disk plus corona system

Details Time dependent accretion onto a black hole in a disk plus corona system Time dependent accretion onto a black hole in a disk plus corona system

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38.2903j&link_type=abstract

Advances in Space Research, Volume 38, Issue 12, p. 2903-2905.

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Hard X-ray lightcurves exhibit delays of ˜1 s with respect to the soft X-ray lightcurves when the microquasar GRS 1915+105 is in the state of frequent, regular outbursts. Such outbursts are supposed to be driven by the radiation pressure instability of the inner disk parts. The hard X-ray delays are then caused by the time needed for the adjustment of the corona to changing conditions in the underlying disk. We support this claim by the computation of the time evolution of the disk, including a non-stationary evaporation of the disk and mass exchange with the corona.

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