The XMM-Newton view of the Galactic Centre
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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.
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
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