Modeling the Dark Matter Halo Properties of Cluster Galaxies

Details Modeling the Dark Matter Halo Properties of Cluster Galaxies Modeling the Dark Matter Halo Properties of Cluster Galaxies

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...201.1302e&link_type=abstract

American Astronomical Society, 201st AAS Meeting, #13.02; Bulletin of the American Astronomical Society, Vol. 34, p.1114

Astronomy and Astrophysics

Astronomy

Scientific paper

Using the Hα rotation curves and I band profiles of over 500 high surface brightness cluster galaxies, we have modeled the disk mass-to-light ratio, dark matter halo central density, and halo core radius. The distribution of the fitted parameters, and dependencies with cluster-centric distance, are presented and discussed. This work is supported by NSF REU site, grant AST 0097356.

Affiliated with

Also associated with

No associations

Rating

Modeling the Dark Matter Halo Properties of Cluster Galaxies 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 Modeling the Dark Matter Halo Properties of Cluster Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the Dark Matter Halo Properties of Cluster Galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1889345