A parsec scale X-ray extended structure from the X-ray binary Circinus X-1

被引:15
|
作者
Soleri, P. [1 ]
Heinz, S. [2 ]
Fender, R. [1 ,3 ]
Wijnands, R. [1 ]
Tudose, V. [1 ,4 ,5 ]
Altamirano, D. [1 ]
Jonker, P. G. [6 ,7 ]
van der Klis, M. [1 ]
Kuiper, L. [6 ]
Kaiser, C. [3 ]
Casella, P. [1 ]
机构
[1] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[2] Univ Wisconsin, Dept Astron, Madison, WI 53705 USA
[3] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England
[4] Acad Romana, Astron Inst, RO-040557 Bucharest, Romania
[5] Res Ctr Atom Phys & Astrophys, RO-077125 Bucharest, Romania
[6] SRON, Netherlands Inst Space Res, NL-3584 CA Utrecht, Netherlands
[7] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
ISM: jets and outflow; stars: individual: Cir X-1; X-rays: binaries; RESOLUTION CAMERA HRC; RELATIVISTIC OUTFLOW; CIR X-1; RADIO; JET; DISCOVERY; STAR; COMPANION; MODEL; AXAF;
D O I
10.1111/j.1745-3933.2008.00574.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of the analysis of two Chandra observations of Circinus X-1 performed in 2007, for a total exposure time of similar to 50 ks. The source was observed with the High Resolution Camera during a long X-ray low-flux state of the source. Cir X-1 is an accreting neutron star binary system that exhibits ultra-relativistic arcsec-scale radio jets and an extended arcmin-scale radio nebula. Furthermore, a recent paper has shown an X-ray excess on arcmin-scale prominent on the side of the receding radio jet. In our images, we clearly detect X-ray structures on both the side of the receding and the approaching radio jet. The X-ray emission is consistent with a synchrotron origin. Our detection is consistent with neutron star binaries being as efficient as black hole binaries in producing X-ray outflows, despite their shallower gravitational potential.
引用
收藏
页码:L1 / L5
页数:5
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