Angular Momentum in Groups from Cosmological Simulations

Details Angular Momentum in Groups from Cosmological Simulations Angular Momentum in Groups from Cosmological Simulations

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..220..477b&link_type=abstract

International Astronomical Union Symposium no. 220, held 21 - 25 July, 2003 in Sydney, Australia. Eds: S. D. Ryder, D. J. Pisano

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Scientific paper

We have performed high resolution cosmological N-body simulations in which halos of 1011 M&sun; are resolved with over 700 particles. We report on the internal structure of group-sized halos (masses between 1011 M&sun; and 1014 M&sun;), particularly on how the angular momentum within the halo correlates with the shape of the halo and with the angular momentum at other radii. We find that many halos have an inner region whose angular momentum is disconnected with that of the outer halo.

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