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X-ray Emission from the Sombrero Galaxy: Discrete Sources

  • Authors: Zhiyuan Li, Lee R. Spitler, Christine Jones, William R. Forman, Ralph P. Kraft, Rosanne Di Stefano, Shikui Tang, Q. Daniel Wang, Marat Gilfanov, and Mikhail Revnivtsev

LI et al. 2010 The Astrophysical Journal 721 1368.

  • Provider: AAS Journals

Caption: Figure 1.

Smoothed 0.4–6 keV intensity images of M104 in panel (a) in the 23′ × 23′ region. Detected X-ray sources are marked with circles of the 90% EER. GC sources are further marked with crosses. The ellipse (8 farcm7 × 3 farcm5) represents the D 25 isophote of the galaxy; the large circle encloses sources of interest; (b) the 10′ × 10′ region. The two dashed ellipses outline the dust lane and (c) the central 1 farcm5 × 1 farcm5 region.

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