Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006–2007 outburst

M. Raiteri, C.; Villata, M.; M. Larionov, V.; F. Aller, M.; Bach, U.; Gurwell, Mark; M. Kurtanidze, O.; Lähteenmäki, A.; Nilsson, K.; E. Volvach, A.; D. Aller, H.; A. Arkharov, A.; Bachev, R.; Berdyugin, A.; Böttcher, M.; S. Buemi, C.; Calcidese, P.; Cozzi, Emanuele; Di Paola, A.; Dolci, M.; H. Fan, J.; Forné, E.; Foschini, L.; C. Gupta, Alok; A. Hagen‐Thorn, V.; Hooks, L.; Hovatta, T.; Joshi, M.; Kadler, M.; N. Kimeridze, G.; S. Konstantinova, T.; Kostov, A.; P. Krichbaum, T.; Lanteri, L.; V. Larionova, L.; Lee, Chung‐Uk; Leto, P.; Lindfors, E.; Montagni, F.; Nesci, R.; Nieppola, E.; G. Nikolashvili, M.; Ohlert, J.; Oksanen, A.; Ovcharov, E.; Pääkkönen, Pertti; Pasanen, M.; Pursimo, T.; Agramunt, J.; Semkov, E.

doi:10.1051/0004-6361:20079044

Public

Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the 2006–2007 outburst

Shared by NobleBlocks on Jan 9, 2008 • 12:00 AM UTC

Authors:

C. M. Raiteri

M. Villata

V. M. Larionov

Abstract

Context.The blazar AO 0235+164 was claimed to show a quasi-periodic behaviour in the radio and optical bands in the past, with the main outbursts repeating every 5–6 years. However, the predicted 2004 outburst did not occur, and further analysis suggested a longer time scale, according to which the ...

Subject

Blazar

Physics

Astrophysics

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