CYG X-1 spectral variability observed with RXTE and BATSE/CGRO

Details CYG X-1 spectral variability observed with RXTE and BATSE/CGRO CYG X-1 spectral variability observed with RXTE and BATSE/CGRO

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.4305s&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #43.05; Bulletin of the American Astronomical Society, Vol. 30, p.1313

Astronomy and Astrophysics

Astronomy

Scientific paper

Hard X-ray spectral variability is important for understanding the high energy emission mechanism in X-ray binary black hole candidates. The canonical black hole candidate Cyg X-1 was observed extensively in various states with RXTE and CGRO/BATSE. We report our analysis of Cyg X-1 hard X-ray spectral variations during these observations, with special attention to the correlations between the power-law index, the power-law cutoff energy, the reflection component, and the hard X-ray flux in various intensity states.

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