The structure and emission model of the relativistic jet in the quasar 3C 279 inferred from radio to high-energy [gamma]-ray observations in 2008-2010

The structure and emission model of the relativistic jet in the quasar 3C 279 inferred from radio to high-energy [gamma]-ray observations in 2008-2010

We present time-resolved broadband observations of the quasar 3C 279 obtained from multi-wavelength campaigns conducted during the first two years of the Fermi Gamma-ray Space Telescope mission. While investigating the previously reported γ-ray/optical flare accompanied by a change in optical polari...

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Bibliographic Details
Main Authors: Hayashida, M., Madejski, G., Nalewajko, K., Sikora, M., Wehrle, A., Ogle, P., Collmar, W., Larsson, S., Fukazawa, Y., Itoh, R., Chiang, J., Stawarz, L., Blandford, R., Richards, J., Max-Moerbeck, W., Readhead, A., Buehler, R., Cavazzuti, E., Ciprini, S., Gehrels, N., Reimer, A., Szostek, A., Tanaka, T., Tosti, G., Uchiyama, Y., Kawabata, K., Kino, M., Sakimoto, K., Sasada, M., Sato, S., Uemura, M., Yamanaka, M., Greiner, J., Kruehler, T., Rossi, A., Macquart, Jean-Pierre, Bock, D., Villata, M., Raiteri, C.
Format: Journal Article
Published: Institute of Physics Publishing, Inc. 2012
Online Access:http://hdl.handle.net/20.500.11937/46364

Internet

http://hdl.handle.net/20.500.11937/46364

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