Processes behind the keV-TeV Connection in Galactic Jet Sources

Details Processes behind the keV-TeV Connection in Galactic Jet Sources Processes behind the keV-TeV Connection in Galactic Jet Sources

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confr..37b&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 37-37"

Physics

Scientific paper

X-ray binaries with relativistic jets can produce very energetic radiation. The likely occurrence of shocks, and the presence of dense matter, magnetic and photon fields, render these sources very good candidates to produce non-thermal radiation, as shown by observations. In the X-ray and TeV domains, it is common to look for correlations in the emission at both energy ranges due to a likely physically linked origin: synchrotron/IC emission in leptonic models, neutral pion gamma-rays/secondary radiation in hadronic ones. We review here different mechanisms that encompass these keV--TeV connection to explore the radiation processes in galactic jet sources.

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