Fig. 2
a) RGB image of VCC 1249 obtained combining the NGVS images in the u,g,z filters. The outlying H ii regions studied in this work are highlighted. Contamination from the light associated with the halo of M 49 is clearly visible. b) RGB image of VCC 1249 obtained after subtracting a model for the light distribution in M 49. c) NUV contours superposed on the RGB image of VCC 1249, after subtracting M 49. d) Enlargement of the region enclosed in the dashed yellow box in panel b). Faint blue structures are visible near the highlighted H ii regions.
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