Fig. 11
Comparison of the relative differences of slope (m) and Y-intercept (C0) values obtained from the linear fits performed to the barred galaxies vs. those performed to the unbarred galaxies in the photometric planes of Type-III galaxies being studied. Left: trends for the R-band data by E08 and G11. Right: trends for the 3.6 μm data by L14. See the caption and legend of Fig. 10.
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