Large-scale, decelerating, relativistic X-ray jets from the microquasar XTE J1550-564

被引:219
作者
Corbel, S [1 ]
Fender, RP
Tzioumis, AK
Tomsick, JA
Orosz, JA
Miller, JM
Wijnands, R
Kaaret, P
机构
[1] Univ Paris 07, F-75221 Paris 05, France
[2] Ctr Etud Saclay, CEA, Serv Astrophys, F-91191 Gif Sur Yvette, France
[3] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands
[4] Ctr High Energy Astrophys, NL-1098 SJ Amsterdam, Netherlands
[5] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[6] Univ Calif San Diego, Ctr Astrophys & Space Sci, La Jolla, CA 92093 USA
[7] Univ Utrecht, Astron Inst, NL-3508 TA Utrecht, Netherlands
[8] MIT, Ctr Space Res, Cambridge, MA 02139 USA
[9] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
D O I
10.1126/science.1075857
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
We have detected, at x-ray and radio wavelengths, large-scale moving jets from the microquasar XTE J1550-564. Plasma ejected from near the black hole traveled at relativistic velocities for at least 4 years. We present direct evidence for gradual deceleration in a relativistic jet. The broadband spectrum of the jets is consistent with synchrotron emission from high-energy (up to 10 tera-electron volts) particles that were accelerated in the shock waves formed within the relativistic ejecta or by the interaction of the jets with the interstellar medium. XTE J1550-564 offers a rare opportunity to study the dynamical evolution of relativistic jets on time scales inaccessible for active galactic nuclei jets, with implications for our understanding of relativistic jets from Galactic x-ray binaries and active galactic nuclei.
引用
收藏
页码:196 / 199
页数:4
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