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Fig. 5


Two-color image toward G20.0-0.2 in Galactic coordinates. In red with contours: emission of the 13CO integrated every 1.05 km s-1 in the velocity range between 62 km s-1 and 71 km s-1 (contour levels are 2.7, 4.0, and 5.3 K km s-1). In green: radio continuum emission of G20 at 20 cm. We have marked the two molecular clumps A and B that form the MC probably interacting with the SNR. A third clump (C) appears in the direction of the flattest border of G20 but is not in contact with the remnant.

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