The changing look of PKS 2149-306

被引:14
作者
Bianchin, V. [1 ]
Foschini, L. [1 ]
Ghisellini, G. [2 ]
Tagliaferri, G. [2 ]
Tavecchio, F. [2 ]
Treves, A. [3 ]
Di Cocco, G. [1 ]
Gliozzi, M. [4 ]
Pian, E. [5 ]
Sambruna, R. M. [6 ]
Wolter, A. [2 ]
机构
[1] INAF IASF Bologna, I-40129 Bologna, Italy
[2] Osserv Astron Brera, INAF, I-23807 Merate, Italy
[3] Univ Insubria, Dipartimento Sci, Como, Italy
[4] George Mason Univ, Fairfax, VA 22030 USA
[5] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[6] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
关键词
quasars: individual: PKS 2149-306; quasars: general; X-rays: galaxies; RADIO-LOUD QUASARS; ACTIVE GALACTIC NUCLEI; HIGH-REDSHIFT QUASARS; XMM-NEWTON OBSERVATIONS; PHOTON IMAGING CAMERA; X-RAY-SPECTRA; EMISSION-LINE; TELESCOPE; BLAZARS; CATALOG;
D O I
10.1051/0004-6361/200811128
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We study the blazar nature of the high-redshift Flat-Spectrum Radio Quasar PKS 2149-306 (z = 2.345) by investigating its long-term behavior. Methods. We analyzed all publicly available optical-to-X-ray observations performed by XMM-Newton, Swift, and INTEGRAL. Results. PKS 2149-306 is one of four blazars at z > 2 that have been observed in the hard-X-ray regime with both the BAT and ISGRI instruments. Observations acquired almost 1 year apart in the 60-300 keV energy band in the object rest frame, exhibit no noticeable change in spectral slope associated with a flux variation of more than a factor of two. Swift data appear to show a roll-off below similar to 1 keV, which becomes increasingly evident during a similar to 3-day time-frame, that can be explained as the natural spectral break caused by the Inverse Compton onset. The broad-band spectra allow us to identify two different states. The SED modeling suggests that they can be interpreted by only a change in the bulk Lorentz factor of the jet.
引用
收藏
页码:423 / 428
页数:6
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