Probing the shot behaviour in Cygnus X-1 using simultaneous AstroSat-NICER observation

We analyse the aperiodic flaring features, also known as shots, observed in Cyg X-1 in the 0.1-80 keV energy band using a 6.39 ks simultaneous observation with AstroSat and Neutron star Interior Composition ExploreR (NICER). We detect 49 simultaneous shots in the soft and hard X-ray bands with NICER and AstroSat-LAXPC, respectively. We observe the shot profile for the first time in soft X-rays (0.1-3 keV), which shows a spectral peak at similar to 2 keV. Using time-averaged spectroscopy, we measured the truncation of the inner accretion disc at 6.7 +/- 0.2 gravitational radii. The shot-phase-resolved spectroscopy allowed us to identify the origin of some of the brightest aperiodic peaks in the soft X-rays. We find that the accretion rate is consistent with a constant during the shots while the inner edge of the accretion disc moves inwards/outwards as these shots rise/decay. We discuss the possible mechanisms causing the swing in the inner radius.

Automated summary

This study analyses the aperiodic flaring features observed in Cyg X-1, measuring the truncation of the inner accretion disc and studying the movement of the inner edge. The research discusses possible mechanisms causing these phenomena.