星暴星系m82和ngc253的非热辐射

Yoel Rephaeli , Massimo Persic
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引用次数: 3

摘要

探测到附近的星暴星系m82和NGC 253的高能γ射线发射,首次在银河系外的非agn环境中建立了轻子和强子过程之间的直接联系。我们回顾了这些过程中最相关的方面,并将理论预测与现有的无线电和γ射线测量结果进行了对比,以确定这些星系中的粒子光谱特性和能量密度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Nonthermal Emission in the Starburst Galaxies M 82 & NGC 253

Detection of high-energy γ-ray emission from the nearby starburst galaxies M 82 and NGC 253 establishes, for the first time, a direct link between leptonic and hadronic processes in an extragalactic non-AGN environment. We review the most relevant aspects of these processes and contrast theoretical predictions with available radio and γ-ray measurements in order to determine the particle spectral properties and energy densities in these galaxies.

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