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Fig. 6

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Molecular clouds in the vicinity of N132D. The image shows the CO emission (color scale in K km s−1) from the MAGMA survey (Wong et al. 2011)5. White contours denote Chandra X-ray emission from N132D6 (Borkowski et al. 2007). The best-fit position of the gamma-ray emission is denoted by the cross, and the elliptical contours are the confidence regions of the position at 2 and 3σ. The dashed circle illustrates the 99% CL UL on the extension established at 3.3′. The scale bar indicates 1′.

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