Fig. 14
Five simulation models from Salo & Laurikainen (2016) are shown at five different galaxy inclinations. The models differ in the bulge-to-disk mass ratio, which varies from B/D = 0.01 to B/D = 0.16. The labels in the frames for i = 30°–75° indicate the mean and standard deviation of B4 for the B/P/X/bl feature, measured from the region between the two marked isophotes.
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