Corbel S, Fender R P, Tzioumis A K, Tomsick J A, Orosz J A, Miller J M, Wijnands R, Kaaret P
Université Paris VII and Service d'Astrophysique, Commissariat à l'Energie Atomique CE-Saclay, 91191 Gif sur Yvette, France.
Science. 2002 Oct 4;298(5591):196-9. doi: 10.1126/science.1075857.
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.
我们已经在X射线和射电波段探测到来自微类星体XTE J1550 - 564的大规模移动喷流。从黑洞附近喷出的等离子体以相对论速度行进了至少4年。我们提供了相对论性喷流逐渐减速的直接证据。喷流的宽带光谱与高能(高达10万亿电子伏特)粒子的同步辐射发射一致,这些粒子是在相对论性抛射物内部形成的冲击波中或通过喷流与星际介质的相互作用而加速的。XTE J1550 - 564提供了一个难得的机会,可在活动星系核喷流无法企及的时间尺度上研究相对论性喷流的动力学演化,这对我们理解银河系X射线双星和活动星系核的相对论性喷流具有重要意义。