Fig. 17
Distribution of “projected” axis ratios and rotational velocity for 100 random inclinations at intervals separated by 1 Gyr during each of the simulation runs, compared to galaxies with vrot = 0.5 × w50 ≤ 100 km s-1 from the catalog of nearby galaxies (Karachentsev et al. 2004) (gray). Darker colors indicare a higher density of objects in this plane.
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