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首页> 外文期刊>PASJ: Publications of the Astronomical Society of Japan >Galactic Center threads as nuclear magnetohydrodynamic waves
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Galactic Center threads as nuclear magnetohydrodynamic waves

机译:银河中心螺纹作为核磁流动动力学波

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摘要

Propagation of fast-mode magnetohydrodynamic (MHD) compression waves is traced in the Galactic Center with a poloidal magnetic cylinder. MHD waves ejected from the nucleus are reflected and guided along the magnetic field, exhibiting vertically stretched fronts. The radio threads and non-thermal filaments are explained as due to tangential views of the waves driven by sporadic activity in Sgr A*, or by multiple supernovae. In the latter case, the threads could be extremely deformed relics of old supernova remnants exploded in the nucleus.
机译:快速模式磁力动力学(MHD)压缩波的传播在半乳液中心追踪,具有粒状中心。 从核中弹出的MHD波被沿磁场反射和引导,呈现垂直拉伸的前线。 由于在SGRA *的散散活动驱动的波的变形视图,或者由多个超新星引起的波浪的切向视图。 在后一种情况下,线程可能是在核中爆炸的旧超新星残余物的极其变形的遗物。

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