Multi-frequency monitoring of γ-ray loud blazars

Authors :: Bach, U.
Raiteri, C. M.
Villata, M.
Fuhrmann, L.
Buemi, C. S.
Larionov, V. M
Leto, P.
Arkharov, A. A.
Coloma, J. M.
Di Paola, A.
Dolci, M.
Efimova, N.
Forné, E.
Ibrahimov, M. A.
Hagen-Thorn, V.
Konstantinova, T.
Kopatskaya, E.
Lanteri, L.
Kurtanidze, O. M.
Maccaferri, G.
Nikolashvili, M. G.
Orlati, A.
Ros, J. A.
Tosti, G.
Trigilio, C.
Umana, G.
Bach, U.
Raiteri, C. M.
Villata, M.
Fuhrmann, L.
Buemi, C. S.
Larionov, V. M
Leto, P.
Arkharov, A. A.
Coloma, J. M.
Di Paola, A.
Dolci, M.
Efimova, N.
Forné, E.
Ibrahimov, M. A.
Hagen-Thorn, V.
Konstantinova, T.
Kopatskaya, E.
Lanteri, L.
Kurtanidze, O. M.
Maccaferri, G.
Nikolashvili, M. G.
Orlati, A.
Ros, J. A.
Tosti, G.
Trigilio, C.
Umana, G.
Source :: Astronomy and Astrophysics; March 2007, Vol. 464 Issue: 1 p175-186, 12p
Publication Year :: 2007
Abstract: Context.Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ultimately, how the energy is extracted from the central black hole in radio-loud active galactic nuclei.

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