gamma-Ray Generation in Microquasars: the link with AGN

gamma-Ray Generation in Microquasars: the link with AGN

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 t...

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Hauptverfasser: Latham, I J, Aye, K-M, Brown, A M, Chadwick, P M, Hadjichristidis, C N, Le Gallou, R, McComb, T J L, Nolan, S J, Orford, K J, Osborne, J L, Noutsos, A, Rayner, S M
Format: Tagungsbericht
Sprache:eng
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Zusammenfassung: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.
ISSN:0094-243X
DOI:10.1063/1.1878424