Multiwavelength studies of Galactic black holes using INTEGRAL

Details Multiwavelength studies of Galactic black holes using INTEGRAL Multiwavelength studies of Galactic black holes using INTEGRAL

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.459..211s&link_type=abstract

In: Exploring the gamma-ray universe. Proceedings of the Fourth INTEGRAL Workshop, 4-8 September 2000, Alicante, Spain. Editor:

Physics

1

Accretion, Accretion Disks, Black Hole Physics, Gamma Rays: Observations, X Rays: Stars, Radio Continuum: Stars

Scientific paper

We give a very brief summary of our recent multiwavelength spectral and energy dependent variability studies of the Galactic black hole candidates GRS 1758-258, GX 339-4, Cygnus X-1, 1E 1740.7-2942, and GRS 1915+105. The energy dependent variability behavior of Cygnus X-1 is highlighted. It is shown that this does not depend on the orbital phase, but may be related to longer periods in the binary system. INTEGRAL will play a key role in future studies of these and similar sources because of its ability to simultaneously study the optical through gamma-ray spectrum in detail, because it has good time resolution for studying the variability, and because its imaging capabilities will reduce the problems of confusing sources and background subtraction.

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