论文标题

SS 433的Eastern Jet的硬X射线发射为W50``Manatee''星云供电:粒子重新加速的证据

Hard X-ray emission from the eastern jet of SS 433 powering the W50 `Manatee' nebula: Evidence for particle re-acceleration

论文作者

Safi-Harb, Samar, Mac Intyre, Brydyn, Zhang, Shuo, Pope, Isaac, Zhang, Shuhan, Saffold, Nathan, Mori, Kaya, Gotthelf, Eric V., Aharonian, Felix, Band, Matthew, Braun, Chelsea, Fang, Ke, Hailey, Charles, Nynka, Melania, Rho, Chang D.

论文摘要

我们提出了由Microquasar SS 433提供动力的复杂区域W50(“海牛星云”)的宽带X射线研究,为几个重要的天体物理过程提供了测试床。 The W50 nebula, a Galactic PeVatron candidate, is classified as a supernova remnant but has an unusual double-lobed morphology likely associated with the jets from SS 433. Using NuSTAR, XMM-Newton, and Chandra observations of the inner eastern lobe of W50, we have detected hard non-thermal X-ray emission up to $\sim$30 keV, originating from a几乎没有Arcminute尺寸的打结区域(“头”),位于$ \ Lessim $ 18 $^{\ prime} $(29 PC(29 PC,距离SS 433的距离为5.5 kpc),并将其光子指数限制为1.58 $ \ pm $ 0.05(0.5-30 kev band)。该索引逐渐向东陡峭地向东陡峭地向东倾斜到无线电“耳朵”,其中温度$ kt $ kt $ \ sim $ 0.2 kev占主导地位的热软X射线发射。硬X射线结标记了射流中加速度位置的位置,并需要$ \ gtrsim $ 12 $μ$ g的均衡磁场。从“头部”区域的异常硬光谱指数挑战了经典的粒子加速过程,并指出了亚相关性SS 433射流中的颗粒注入和重新加速,如Blazars和Pulsar风星号所示。

We present a broadband X-ray study of W50 (`the Manatee nebula'), the complex region powered by the microquasar SS 433, that provides a test-bed for several important astrophysical processes. The W50 nebula, a Galactic PeVatron candidate, is classified as a supernova remnant but has an unusual double-lobed morphology likely associated with the jets from SS 433. Using NuSTAR, XMM-Newton, and Chandra observations of the inner eastern lobe of W50, we have detected hard non-thermal X-ray emission up to $\sim$30 keV, originating from a few-arcminute size knotty region (`Head') located $\lesssim$ 18$^{\prime}$ (29 pc for a distance of 5.5 kpc) east of SS 433, and constrain its photon index to 1.58$\pm$0.05 (0.5-30 keV band). The index gradually steepens eastward out to the radio `ear' where thermal soft X-ray emission with a temperature $kT$$\sim$0.2 keV dominates. The hard X-ray knots mark the location of acceleration sites within the jet and require an equipartition magnetic field of the order of $\gtrsim$12$μ$G. The unusually hard spectral index from the `Head' region challenges classical particle acceleration processes and points to particle injection and re-acceleration in the sub-relativistic SS 433 jet, as seen in blazars and pulsar wind nebulae.

扫码加入交流群

加入微信交流群

微信交流群二维码

扫码加入学术交流群,获取更多资源