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Fig. 4


Detection of X-rays emission with Chandra. The observations were smoothed to a resolution of 15. Contours are drawn every 0.35 counts/arcsec2 starting at 0.35 counts/arcsec2. The galaxy center is marked as A. The dashed ellipse shows the 2′′ × 2′′ region around position B which was used to calculate a signal-to-noise of 2.2σ (see Sect. 2.3 for discussion).

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