Physics
Scientific paper
Jul 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2525l&link_type=abstract
Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I
Physics
Scientific paper
We investigate the link between the physical processes, which are responsible for high energy emission from relativistic jets in AGN and micro quasars. We are producing a model based on an existing inhomogeneous, synchrotronself-Compton (SSC) model [3, 4], designed for AGN, to predict gamma-ray emission from relativistic jets in micro quasars. Initially this concentrates on the SSC process but will later include inverse Compton scattering of the photon fields produced by the companion star and the accretion disk. supported by future gamma-ray observations of these objects, with e.g. the H.E.S.S. telescope array, links between the physical processes in the two morphologically similar objects can be made.
Aye Klaus-Michael
Chadwick Paula M.
Hadjichristidis C. N.
Latham I. J.
Le Gallou Roland
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