Radio Observations and Modeling of Supernova Remnants

当超新星的喷出物膨胀时， 进入周围的星际介质，压缩它， 这种膨胀和混合是非常复杂的。 首席研究员建议在附近观察和绘制地图 超新星遗迹，并对它们进行计算机建模。 目标 是增加我们对物理过程的理解， 在他们的地方，特别是要找出如何和在哪里 同步加速器无线电发射发生在他们和如何这 排放随时间变化。

Supernova remnants result when the ejecta of a supernova expands into the ambient interstellar medium, compresses it, and mixes with it. This expansion and mixing are extraordi.narily complex. The Principal Investigator proposes to observe and map nearby supernova remnants and to model them computa.tionally. The goal is to increase our understanding of the physical processes taking place in them, in particular to find out how and where synchrotron radio emission takes place in them and how this emission varies with time.