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Fig. 2


Logarithmically scaled Chandra HRC-I images of the innermost of M 31 combining all observations of 2007/8 (left panel) and 2008/9 (right panel). The images were not binned (HRC electronic pixel size = ) but were smoothed with a Gaussian of FWHM . The X-ray counterparts of novae in the field are marked with black circles.

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