Fig. 6
NGVS g image of VCC 1249 (bottom-left) and of M 49 (top-center) on which the NUV contours (red) and the H i contours taken from McNamara et al. (1994) (yellow) are superposed (the coordinates are precessed from B1950 originally used, to J2000). Note that the peak of the H i cloud nearly coincides with the peak of the NUV emission at the position of the region C2 (LR1 in Lee et al. 2000).
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