The Geometry Of The Filamentary Environment Of Galaxy Clusters

Details The Geometry Of The Filamentary Environment Of Galaxy Clusters The Geometry Of The Filamentary Environment Of Galaxy Clusters

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21720406n&link_type=abstract

American Astronomical Society, AAS Meeting #217, #204.06; Bulletin of the American Astronomical Society, Vol. 43, 2011

Astronomy and Astrophysics

Astronomy

Scientific paper

We construct filament catalogues in a 250 Mpc/h N-body simulation using the halo based filament finder of Zhang et al.(2009) to study the properties of filaments in cluster neighborhood. We consider the cluster environment (within 10 Mpc/h spheres) in part because the finder does so. We find the filaments attached to the cluster tend to lie within a 3 Mpc/h thick plane, although often at least one filament lies outside the plane. For many clusters, this planar geometry has a correlation with the line of sight dependent mass scatter in several observables.

Affiliated with

Also associated with

No associations

Rating

The Geometry Of The Filamentary Environment Of Galaxy Clusters 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 The Geometry Of The Filamentary Environment Of Galaxy Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Geometry Of The Filamentary Environment Of Galaxy Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1396822