We study the dark and luminous mass distributions, circular velocity curves (CVCs), lineof-sight kinematics and angular momenta for a sample of 42 cosmological zoom simulations of galaxies with stellar masses from 2.0 10 10 to 3.4 10 11 M h -1 . Using a temporal smoothing technique, we are able to reach large radii. We find the following.
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Wu et al. (2014) studied this question.
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