Inproceedings,

Spin Flips: Variation in the Orientation of Dark Matter Halos Over Their Merger Histories

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HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION, 1240, page 403--404. AIP, (Jun 8, 2010)
DOI: 10.1063/1.3458546

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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