大尺度射流/介质相互作用
Jet/medium interactions at large scales
摘要：
在银河系和河外喷流与周围介质的相互作用部位都可以产生高能辐射。我们已经开发了一个辐射模型，占连续注入的相对论性电子的正向，反向和再校准的冲击中开发的壳，茧和refinenation相互作用区域，分别。我们还进行了流体动力学模拟，以建立在银河系和河外系统的物理特性。由此产生的非热发射的研究假设不同的值的喷流功率，外部质量密度和源年龄的FR I星系和银河系微类星体。所获得的通量进行比较，在无线电，X射线和伽马射线波段的电流仪器的灵敏度。
英文摘要：
High energy emission can be produced in the interaction sites of both galactic and extragalactic jets with the surrounding medium. We have developed a radiative model that accounts for the continuous injection of relativistic electrons in the forward, reverse and recollimation shocks developed in the shell, cocoon and reconfinement interaction regions, respectively. We also performed hydrodynamical simulations to establish the physical properties in both galactic and extragalactic systems. The resulting non-thermal emission is studied assuming different values for the jet power, the external mass density and the source age for both FR I galaxies and galactic microquasars. The obtained fluxes are compared to current instrument sensitivities at radio, X-ray and gamma-ray bands.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
