Energy-dependent X-ray variability of Cygnus X-1

Details Energy-dependent X-ray variability of Cygnus X-1 Energy-dependent X-ray variability of Cygnus X-1

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..aprx11004s&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Galactic Black Hole Candidate Cygnus X-1 exhibits unusual rapid X-ray variability properties. In particular, the evolution of the energy-dependence of the variability cannot be explained by simple models of the source. Here we will discuss our ongoing study of the data taken by the Rossi X-ray Timing Explorer, and the implications that this has on the accretion disk models.

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