The Baryonic Bar and the Triaxiality of the Dark Matter Halo

Details The Baryonic Bar and the Triaxiality of the Dark Matter Halo The Baryonic Bar and the Triaxiality of the Dark Matter Halo

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374..497m&link_type=abstract

From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer

Mathematics

Logic

Scientific paper

The halo structure, generated by the cosmology, which is far from stability and isotropy, plays a crucial role in triggering and fueling long living bars in disks with negligible self-gravity, i.e., dark matter (DM) dominated disks. However, the effects of the fully cosmological frame-work, i.e., of the environment, cannot be neglected in the evolution of the more massive disks. The bar cannot destroy the halo triaxiality which always restores its initial value, also when the bar disappears.

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