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UGC 11332 (NGC 6654A). There is a good agreement between our H{alpha} map and that of James et al. (2004). However, our image is affected by very bad seeing conditions (see Table C2) resulting in a diffuse emission around the galaxy that is most probably an artefact. No H I velocity map is available in the literature. The width of the H I profile at 20 per cent (331 km s^-1^ from Springob et al. 2005, 315 km s^-1^ from Bottinelli et al. 1990) is significantly larger than our H{alpha} velocity field amplitude (about 200 km s^-1^), suggesting that our H{alpha} velocity field does not reach the maximum rotation velocity althougH It extends up to the optical radius. Anonymous Sm of very low surface brightness at 2.5 arcmin north-preceding. {NGC 6654A in RC1. H. Corwin} Blue, several bright patches Late spiral? See UGC 11331 See Ap. J., 82, 74, 1935 and Ap. J., 85, 325, 1937. There is an anonymous Sm galaxy of very low surface brightness at 2.5 arcmin north-preceding. |