Radio and infrared study of the supernova remnant candidate HESS J1912+101

Open Access

Fig. 5

Two-color image of the infrared emission toward HESS J1912+101: 8.0 μm (in red) and 24.0 μm (in green). The white contours are the TeV emission, and the yellow rectangle is a zoomed-in view of the area shown in Fig. 6. Red crosses are the radio sources of Fig. 1.

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