超新星残骸的无线电频谱变化

2009 13th International Symposium on Antenna Technology and Applied Electromagnetics and the Canadian Radio Science Meeting Pub Date : 2009-03-24 DOI:10.1109/ANTEMURSI.2009.4805087

D. Leahy, T. Wenwu

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引用次数: 0

摘要

超新星遗迹是我们银河系内天文射电辐射的主要来源。其机理是相对论电子的同步辐射，观测到的谱取决于相对论电子谱和从源到观测者的传播效应。这里讨论了电子谱和无线电吸收效应，并与最近观测到的银河系超新星遗迹进行了比较。

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Radio spectrum variations in supernova remnants

Supernova remnants are prominent sources of astronomical radio emission within our galaxy. The mechanism is synchrotron radiation from relativistic electrons and the observed spectrum depends on the relativistic electron spectrum and propagation effects from the source to the observer. Here the electron spectrum and radio absorption effects are discussed and compared with recent observations of galactic supernova remnants.

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2009 13th International Symposium on Antenna Technology and Applied Electromagnetics and the Canadian Radio Science Meeting

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