Modelling blazar radiation spectra Electron injection break and pair content of quasar jets

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dc.creatorBlazejowski, M.
dc.creatorSikora, M.
dc.creatorModerski, R.
dc.creatorBulik, T.
dc.date1999-10-22
dc.date.accessioned2026-07-07T02:34:00Z
dc.date.available2026-07-07T02:34:00Z
dc.descriptionWe study the dependence of nonthermal radiation spectra in OVV quasars on location of the low energy break in the electron/positron injection function. We show that the high energy spectra produced during the outbursts are presumably superposed from two components, one resulting from Comptonization of emission lines, which dominates at MeV-GeV energies, and the other resulting from Comptonization of infrared radiation, which dominates in the X-ray band.
dc.description4 pages, to appear in the proceedings of the Bologna Conference on "X-ray Astronomy 1999: Stellar Endpoints, AGNs and the Diffuse X-ray Background" (Astroph. Lett. and Comm.)
dc.identifierhttps://arxiv.org/abs/astro-ph/9910416
dc.identifierhttp://arxiv.org/abs/astro-ph/9910416
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15074
dc.subjectAstrophysics
dc.titleModelling blazar radiation spectra Electron injection break and pair content of quasar jets
dc.typetext

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