dc.contributor.author |
Ghosh, K. K |
|
dc.contributor.author |
Ramsey, B. D |
|
dc.contributor.author |
Sivaram, C |
|
dc.date.accessioned |
2008-08-14T05:46:55Z |
|
dc.date.available |
2008-08-14T05:46:55Z |
|
dc.date.issued |
1999-06 |
|
dc.identifier.citation |
Astroparticle Physics, Vol. 11, No. 1 - 2, pp. 69 - 71 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/3123 |
|
dc.description.abstract |
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. |
en |
dc.format.extent |
194220 bytes |
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dc.format.mimetype |
application/pdf |
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dc.language.iso |
en |
en |
dc.publisher |
Elsevier Science B. V |
en |
dc.relation.uri |
http://dx.doi.org/10.1016/S0927-6505(99)00028-6 |
en |
dc.subject |
Gamma-ray |
en |
dc.subject |
UV Photons |
en |
dc.title |
Origin of MeV gamma-ray emissions from blazars |
en |
dc.type |
Article |
en |