X-Ray Spectral Variability in Cygnus X-1

Abstract

Spectral variability in different energy bands of X-rays from Cyg X-1 in different states is studied with RXTE observations and time domain approaches. In the hard tail of energy spectrum above $\sim 10$ keV, average peak aligned shots are softer than the average steady emission and the hardness ratio decreases when the flux increases during a shot for all states. In regard to a soft band lower $\sim 10$ keV, the hardness in the soft state varies in an opposite way: it peaks when the flux of the shot peaks. For the hard and transition states, the hardness ratio in respect to a soft band during a shot is in general lower than that of the steady component and a sharp rise is observed at about the shot peak. For the soft state, the correlation coefficient between the intensity and hardness ratio in the hard tail is negative and decreases monotonically as the timescale increases from 0.01 s to 50 s, which is opposite to that in regard to a soft band. For the hard and transition states, the correlation coefficients are in general negative and have a trend of decrease with increasing timescale.

14 pages, 3 figures, accepted by ApJ

References in corpus (4)

• Long Term Variability of Cyg X-1 I. X-ray spectral-temporal correlations in the hard state
• Higher Order Variability Properties of Accreting Black Holes
• Short Timescale Correlations Between Line and Continuum Fluxes in Cygnus X-1
• Diagnostics of Neutron Star and Black Hole X-Ray Binaries with X-Ray Shot Widths

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• X-Ray Spectral Variability in Initial Rise of XTE J1550-564
• Shot cutoff timescales in different spectral states of Cygnus X-1