γ-Ray Generation in Microquasars: the link with AGN

Details γ-Ray Generation in Microquasars: the link with AGN γ-Ray Generation in Microquasars: the link with AGN

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..323l&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

Galactic Nuclei, Circumnuclear Matter, And Bulges, Quasars, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The link between the physical processes responsible for high energy emission from relativistic jets in AGN and microquasars is investigated. A Fortran code based on an existing inhomogeneous, synchrotron self-Compton (SSC) model, for AGN is presented. The code is then applied to the AGN 3C 279 and the microquasar LS5039. Spectral energy distributions (SED's) are presented.

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