{ "id": "0909.5057", "version": "v1", "published": "2009-09-28T10:37:18.000Z", "updated": "2009-09-28T10:37:18.000Z", "title": "Gamma-rays from the IC $e^\\pm$ pair cascade in the radiation field of an accretion disk: Application to CenA", "authors": [ "J. Sitarek", "W. Bednarek" ], "comment": "7 pages, 4 figures, accepted for publication in MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "The very short time scale variability of TeV $\\gamma$-ray emission from active galaxies suggests that the acceleration process of particles and the production of primary $\\gamma$-rays likely occurs relatively close to the accretion disk. We calculate the $\\gamma$-ray spectra produced in an Inverse Compton $e^\\pm$ pair cascade initiated by primary $\\gamma$-rays which are injected close to the surface of the accretion disk. Possible synchrotron energy losses of secondary cascade $e^\\pm$ pairs are also taken into account. Since the soft radiation field is anisotropic, the resulting $\\gamma$-ray spectra strongly depend on the observation angle. We investigate their basic properties for different parameters describing such a model. The model is applied to the misaligned blazar Cen A recently detected in the TeV $\\gamma$-rays. We conclude on the site of the $\\gamma$-ray emission region in Cen A based on the comparison of the model with the observations of this source in the GeV-TeV energy range.", "revisions": [ { "version": "v1", "updated": "2009-09-28T10:37:18.000Z" } ], "analyses": { "keywords": [ "accretion disk", "pair cascade", "short time scale variability", "gamma-rays", "application" ], "tags": [ "journal article" ], "publication": { "doi": "10.1111/j.1365-2966.2009.15785.x", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2010, "month": "Jan", "volume": 401, "number": 3, "pages": 1983 }, "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable", "inspire": 832388, "adsabs": "2010MNRAS.401.1983S" } } }