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Fig. 5


H.E.S.S. smoothed VHE γ-ray excess contours in blue overlaid on the Molonglo 843 MHz map (grey scale, in Jy/beam; Green et al. 1999). Also shown are SNRs (purple, Green 2009), the pulsar PSR J1648–4611 (Manchester et al. 2005), the LMXB 4U 1642–45 (Forman et al. 1978), Fermi-LAT sources (Abdo et al. 2011), the magnetar CXOU J164710.2–455216 (Muno et al. 2006a) as a black upright triangle and the stellar cluster Wd 1.

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