X-ray Properties of Microquasars

Details X-ray Properties of Microquasars X-ray Properties of Microquasars

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..35h&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 35-35"

Physics

Scientific paper

Microquasars, or X-ray binaries which exhibit relativistic jets, are observed extensively at all wavelengths. The accretion disk and corona radiate in the X-rays, while the jets are responsible for the radio emission. In this talk, I will concentrate on the X-ray properties of microquasars, showing results from missions both old and new and I will outline our current understanding of the underlying X-ray emission processes involved.

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