Gamma-ray Loud Binary Systems

Details Gamma-ray Loud Binary Systems Gamma-ray Loud Binary Systems

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..40n&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 40-40"

Physics

Scientific paper

We discuss physical mechanisms of radio-to-TeV gamma-ray emission from gamma-ray loud binary systems. The emission spectrum of such systems can be formed in interaction of a relativistic wind (produced either by a young pulsar or via pair production by gamma rays in the photon field of companion star ) with the wind from companion star. We discuss the possibility to constrain the physical characteristics of the pulsar winds from the multiwavelength observations of such systems.

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