Fig. 13.
Adaptively smoothed, exposure-corrected combined EPIC image of the central parts of NGC 185. The image depicts emission detected over the 0.4 keV to 7.0 keV energy range (scaled with zscale/sinh and 100 smoothing counts). The optically detected sources are represented with filled circles, except objects VIEM 8 and 9 which are indicated with dashed circles.
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