Observational Status of Microquasars in the Radio and Gamma-ray Domain

Details Observational Status of Microquasars in the Radio and Gamma-ray Domain Observational Status of Microquasars in the Radio and Gamma-ray Domain

Aug 2007

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

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

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Some of the very high energy gamma-ray sources detected with the modern generation of Cherenkov telescopes have been identified with previously known X-ray binary systems, which are also radio emitters. In addition, some of the currently unidentified high energy and very high energy sources could be powered by relativistic radio jets from X-ray binaries, i.e., microquasars. Here I summarise the current status of our phenomenological knowledge regarding the radio/gamma-ray emission associated with microquasar X-ray binaries.

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