Fig. 12
Comparison of the relative differences of slope (m) and Y-intercept (C0) values obtained from the linear fits performed to the 3.6 μm data by L14 vs. those obtained from the R-band data by E08 and G11 in the photometric planes relating physical scalelengths under study. Left: trends for the S0 galaxies. Right: trends for spirals. See the caption and legend of Fig. 10.
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