Suzaku studies of microquasars

Details Suzaku studies of microquasars Suzaku studies of microquasars

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..275..242u&link_type=abstract

Jets at all Scales, Proceedings of the International Astronomical Union, IAU Symposium, Volume 275, p. 242-249

Physics

1

Accretion, Accretion Disks - Black Hole Physics - X-Rays: Individual (Gx 339-4, Grs 1915+105)

Scientific paper

We report our recent results from multiwavelengths studies of microquasars, focusing on X-ray data of GX 339-4 and GRS 1915+105 obtained with Suzaku and other observatories. The broad band coverage and high energy resolution achieved with Suzaku (or a combination of Chandra/HETGS and RXTE) enable us to perform the most reliable spectral analysis both on iron-K features and continuum, and thus to best constrain the accretion disk structure of microquasars and its relation to the jet formation at various mass accretion rates.

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