Image Details
Caption: Figure 5.
Bulge contribution fB to the galaxy luminosity in the ﹩W1﹩ band (panel a) and morphological T type (panel b) as a function of the disk scale length hW1 in the ﹩W1﹩ band, and ratio of disk radius to the disk scale length ﹩{{R}_{25}}/{{h}_{W1}}﹩ as a function of morphological T type (panel c).
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