TeV Gamma射线观测与宇宙射线起源III
天体物理学
2007-05-23 v2
摘要
本报告主要致力于物理解释，从HEGRA首创的立体观测技术讲起。回顾了对超新星残余的搜索，论证了需要一致的理论，并概述了该理论的要素。该理论是解释SN 1006和Cas A模型的基础。分析结果首次显示，辐射谱和形态细节与这些物体代表一类疑似银河系源群的概念相吻合。对该源群的持续研究是主要新型γ射线仪器的必由之路。
引用
@article{arxiv.astro-ph/0312585,
title = {TeV Gamma-Ray Observations and the Origin of Cosmic Rays III},
author = {H. J. Voelk},
journal= {arXiv preprint arXiv:astro-ph/0312585},
year = {2007}
}
备注
19 pages, 10 figures, Plenary Talk at the 28th International Cosmic Ray Conference, July 31 - August 7, 2003, in Tsukuba, Japan. To be published 2003 by Universal Academy Press, Inc. - Tokyo, Japan. Changes are in captions of Figs. 3, 7a, and 8b