INTEGRAL observations of the blazar 3C 454.3 in outburst

被引:73
作者
Pian, EP
Foschini, LF
Beckmann, VB
Soldi, SS
Türler, MT
Gehrels, N
Ghisellini, GG
Giommi, P
Maraschi, LM
Pursimo, TP
Raiteri, CM
Tagliaferri, G
Tornikoski, M
Tosti, G
Treves, A
Villata, M
Barr, P
Courvoisier, TJL
Di Cocco, G
Hudec, R
Fuhrmann, L
Malaguti, G
Persic, M
Tavecchio, F
Walter, R
机构
[1] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[2] IASF Bologna, INAF, I-40129 Bologna, Italy
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[4] Univ Maryland Baltimore Cty, Dept Phys, Joint Ctr Astrophys, Baltimore, MD 21250 USA
[5] INTEGRAL Sci Data Ctr, CH-1290 Versoix, Switzerland
[6] Observ Geneva, CH-1290 Sauverny, Switzerland
[7] Osserv Astron Brera, INAF, I-23807 Merate, LC, Italy
[8] ASI Sci Data Ctr, I-00044 Frascati, Italy
[9] Osserv Astron Brera, INAF, I-20121 Milan, Italy
[10] Nord Opt Telescope, Santa Cruz De La Palma 38700, Spain
[11] Osserv Astron Torino, INAF, I-10025 Pino Torinese, TO, Italy
[12] Metsahovi Radio Observ, Kylmala 02540, Finland
[13] Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy
[14] Univ Insubria, Dipartimento Matemat & Fis, I-22100 Como, Italy
[15] European Space Agcy, ESTEC, RSSD, NL-2200 AG Noordwijk, Netherlands
[16] Acad Sci Czech Republ, Inst Astron, CS-25165 Ondrejov, Czech Republic
基金
美国国家航空航天局; 美国国家科学基金会; 日本学术振兴会;
关键词
galaxies : active; X-rays : observations;
D O I
10.1051/0004-6361:200600017
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In Spring 2005, the blazar 3C 454.3 underwent a dramatic outburst at all wavelengths from mm to X-rays. This prompted INTEGRAL observations, accomplished in 15 servations, 15-18 May 2005. The source was detected by the INTEGRAL instruments from 3 to 200 keV in a bright state (similar to 5 x 10(-10) erg s(-1) cm(-2)), at least a factor of 2-3 higher than previously observed. This is one of the brightest blazar detections achieved by INTEGRAL. During the 2.5 days of. INTEGRAL monitoring, we detected a similar to 20% decrease in the hard X-rays (20-40 keV), indicating that we have sampled the decaying part of the flare. The decrease is less apparent in the soft X-rays (5-15 keV). The simultaneous optical variations are weakly correlated with those at soft X-rays, and not clearly correlated with those at hard X-rays. The spectral energy distribution exhibits two components, as typically seen in blazars, which can be modeled with synchrotron radiation and inverse Compton scattering occurring in a region external to the broad line region.
引用
收藏
页码:L21 / L25
页数:5
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