Year: 2007
Type: article
Abstract: Context.In spring 2005 the blazar 3C 454.3 was observed in an unprecedented bright state from the near-IR to the hard X-ray frequencies. A mm outburst peaked in June–July 2005, and it was followed by a flux increase at high radio frequencies.
Source: Astronomy and Astrophysics
Authors: M. Villata, C. M. Raiteri, M. F. Aller, U. Bach, M. A. Ibrahimov, Y. Y. Kovalev, O. M. Kurtanidze, V. M. Larionov, C.-U. Lee, P. Leto, A. Lähteenmäki, K. Nilsson, T. Pursimo, J. A. Ros, N. Sumitomo, A. Volvach, H. D. Aller, A. Arai, C. S. Buemi, J. M. Coloma, V. T. Doroshenko, Yu. S. Efimov, L. Fuhrmann, V. A. Hagen-Thorn, M. Kamada, M. Katsuura, T. Konstantinova, E. Kopatskaya, D. Kotaka, Yu. A. Kovalev, M. Kurosaki, L. Lanteri, L. Larionova, M. G. Mingaliev, S. Mizoguchi, K. Nakamura, M. G. Nikolashvili, S. Nishiyama, K. Sadakane, S. G. Sergeev, L. A. Sigua, A. Sillanpää, R. L. Smart, L. O. Takalo, K. Tanaka, M. Tornikoski, C. Trigilio, G. Umana
Institutions: Osservatorio Astrofisico di Torino, National Institute for Astrophysics, University of Michigan, Max Planck Institute for Radio Astronomy, Academy of Sciences Republic of Uzbekistan, Ulugh Beg Astronomical Institute, P.N. Lebedev Physical Institute of the Russian Academy of Sciences, National Radio Astronomy Observatory, Astro Space Center, Leibniz Institute for Astrophysics Potsdam, Evgeni Kharadze Georgian National Astrophysical Observatory, St Petersburg University, Isaac Newton Institute, Korea Astronomy and Space Science Institute, Nordic Optical Telescope, Osaka Kyoiku University, Crimean Astrophysical Observatory, Osservatorio Astrofisico di Catania, Lomonosov Moscow State University, University of Perugia, Special Astrophysical Observatory
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W4301885367