Structural properties of Dark Matter Halos

Details Structural properties of Dark Matter Halos Structural properties of Dark Matter Halos

1999-10-14

arxiv.org/abs/astro-ph/9910266v2

Astronomy and Astrophysics

Astrophysics

6 pages, 3 figures. Minor typos corrected, conclusions unchanged. To appear in the proceedings of the Marseille IGRAP99 confer

Scientific paper

Using the results of a high mass resolution ($256^{3}$ particles) N-body simulation of a cluster-forming region, we study the statistic $\sigma_{v}-M$ for low mass halos (${\rm M} < 10^{12} {\rm M}_{\sun}$), and we compare it with three theoretical models. At the final redshift halos are well described by the Truncated Isothermal Sphere model recently introduced by Shapiro, Iliev & Raga (1999). We speculate that this is a consequence of the action of tidal fields on galaxy formation within clusters.

Affiliated with

Also associated with

No associations

Rating

Structural properties of Dark Matter Halos does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Structural properties of Dark Matter Halos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structural properties of Dark Matter Halos will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-105616