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Fig. 7

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Top: (FUV – NUV) color as a function of the morphological type for the six group members of the NGC 3933 group. The solid line represents the best linear fit for types T =  −0.5 or later (i.e. spiral galaxies and irregular) in Gil de Paz et al. (2007). Members of LGA groups from Marino et al. (2010) are plotted for comparison (see text). Bottom: NUV-r vs. Mr color–magnitude plot for galaxies in the NGC 3933 group. The Yi et al. (2005) red sequence is shown as a solid line. Early-type galaxies in Marino et al. (2011a) are indicated as black dots (see text).

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