Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-06-18
Astrophys.J.652:L75-L78,2006
Astronomy and Astrophysics
Astrophysics
4 pages, 1 figure, accepted for publication in ApJ Letters
Scientific paper
10.1086/510330
We investigate the orientation of the axes and angular momentum of dark matter halos with respect to their neighboring voids using high resolution N-body cosmological simulations. We find that the minor axis of halos tends to be aligned along the line joining the halo with the center of the void, and that the major axis is perpendicular to this line. However, we find that the angular momentum of halos does not have any particular orientation. These results may provide information about the mechanisms whereby the large-scale structure of the Universe affects galaxy formation and cast light upon the issue of the orientation of galaxy disks with respect to their host halos.
Betancort-Rijo Juan
Cuesta Antonio J.
Klypin Anatoly
Patiri Santiago G.
Prada Francisco
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