Fig. 14
Concentration vs. Petrosian AP Asymmetry for our sample (red text) compared to spheroids, early and late type disks, and irregulars taken from Conselice et al. (2000) and the BCG galaxies from Paper I. To make all labels as readable as possible we omitted the SBS0335–052E measurement from Paper I. The red text indicates the UM number of the respective galaxy.
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