Pair annihilation radiation from relativistic jets in γ-ray blazars.

Details Pair annihilation radiation from relativistic jets in γ-ray blazars. Pair annihilation radiation from relativistic jets in γ-ray blazars.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26as..120c.575b&link_type=abstract

Astronomy and Astrophysics Supplement, v.120, p.575-578

Astronomy and Astrophysics

Astrophysics

8

Quasars: General, Galaxies: Jets, Gamma Rays: Theory, Radiation Mechanisms: Non-Thermal

Scientific paper

The contribution of the pair annihilation process in relativistic electron-positron jets to the γ-ray emission of blazars is calculated. For pair densities >10^9^cm^-3^ in the jet the annihilation radiation will dominate the inverse Compton radiation, and due to its bump-like spectrum may explain reported spectral bumps at MeV energies.

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