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Fig. 1

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Wide-field Infrared Survey Explorer (WISE) RGB image at bands W2 (4.6 μm), W3 (12 μm), and W4 (22 μm) of the shocked gas around the runaway star HD 195592; the radiative heating of the swept-up dust produces the IR emission and traces the bowshock. The 95% location-error circle of the gamma-ray source 2FGL J2030.7+4417 is shown (the 99% countour is outside the figure). The probability countours from gamma-ray sources are model-dependent and they must be taken as indicative only.

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