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Chandra And Xmm–Newton Detection Of Large-Scale Diffuse X-Ray Emission From The Sombrero Galaxy, Z Li, Qd Wang, S Hameed
Chandra And Xmm–Newton Detection Of Large-Scale Diffuse X-Ray Emission From The Sombrero Galaxy, Z Li, Qd Wang, S Hameed
Astronomy Department Faculty Publication Series
We present an X-ray study of the massive edge-on Sa galaxy, Sombrero (M 104; NGC 4594), based on XMM–Newton and Chandra observations. A list of 62 XMM–Newton and 175 Chandra discrete X-ray sources is provided, the majority of which are associated with the galaxy. Spectral analysis is carried out for relatively bright individual sources and for an accumulated source spectrum. At energies ≳2 keV, the source-subtracted X-ray emission is distributed similarly as the stellar K-band light and is primarily due to the residual emission from discrete sources. At lower energies, however, a substantial fraction of the source-subtracted emission arises …