银河中心的 XMM-Newton 观测
天体物理学
2007-05-23 v1
摘要
在 X 射线中，银河中心 (GC) 区域呈现为由漫射热 X 射线和非热 X 射线辐射交织的亮度较高的离散天体构成的复杂结构。我们在 XMM-Newton 银河中心调查中 presenting some new findings, focusing particularly on Sgr A*, Sgr A East, the Radio Arc region, and a newly discovered X-ray non-thermal filament.
关键词
引用
@article{arxiv.astro-ph/0212464,
title = {The XMM-Newton view of the Galactic Centre},
author = {Masaaki Sakano and Robert S. Warwick and Anne Decourchelle},
journal= {arXiv preprint arXiv:astro-ph/0212464},
year = {2007}
}
备注
4 pages, 2 figures, uses shuzenji.sty; Proc. of 'Japan-Germany Workshop on Galaxies and Clusters of Galaxies', 29-31 Oct. 2002, Shuzenji, Japan; Manuscript with full size figures are found in http://www.star.le.ac.uk/~mas/research/paper/#Sakano2002jg