Abstract
Semi-analytic models of galaxy formation typically form the spheroidal components of galaxies ( ” bulges”), solely through galactic major mergers. However, it is possible that non-merger events (e.g. a ” fly-by” by a smaller halo) can perturb a galaxy—halo system sufficiently to form a bulge. We present a preliminary investigation into the frequency of major changes in halo and galaxy spin direction, which could be signatures of such events.
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