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2011

GBM Monitoring of Cyg X-1 During the Recent State Transition

Case, G. L., Baldridge, S., Cherry, M. L. et al.

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Cygnus X-1 is a high-mass x-ray binary with a black hole compact object.

It is normally extremely bright in hard x-rays and low energy gamma rays and resides in the canonical hard spectral state.
Recently, however, Cyg X-1 made a transition to the canonical soft state, with a rise in the soft x-ray flux and a decrease in the flux in the hard x-ray and low energy gamma-ray energy bands.
We have been using the Gamma-Ray Burst Monitor on Fermi to monitor the fluxes of a number of sources in the 8--1000 keV energy range, including Cyg X-1.

GBM Monitoring of Cyg X-1 During the Recent State Transition · Around

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