Origin of MeV gamma-ray emissions from blazars

Details Origin of MeV gamma-ray emissions from blazars Origin of MeV gamma-ray emissions from blazars

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aph....11...69g&link_type=abstract

Astroparticle Physics, Volume 11, Issue 1-2, p. 69-71.

Physics

1

Scientific paper

We have developed a model for MeV emission from blazars that involves the production of MeV gamma-rays through Inverse Compton (IC) scattering of electrons in the blob of a jet, with the UV photons of the accretion disk. The OSSE and the COMPTEL spectra of PKS 0528 + 134 have been fitted with the computed MeV gamma-ray fluxes of the above model. A good fit was obtained with electrons of Lorentz factor of 10^1.5 to 10^3 and a jet with viewing angle of <=15^∘ and an accretion disk temperature in the range of 2.0 to 6.0 x10^5 K.

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