The XMM-Newton view of the Galactic Centre
Astrophysics
2007-05-23 v1
Abstract
In X-rays, the Galactic Centre (GC) Region appears as a complex of diffuse thermal and non-thermal X-ray emission intermixed with a population of luminous discrete sources. Here we present some new findings from the XMM-Newton GC survey, focusing particularly on Sgr A*, Sgr A East, the Radio Arc region, and a newly discovered X-ray non-thermal filament.
Cite
@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}
}
Comments
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