Clusters of galaxies compared with N-body simulations - The set of separation vectors

Details Clusters of galaxies compared with N-body simulations - The set of separation vectors Clusters of galaxies compared with N-body simulations - The set of separation vectors

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84...50s&link_type=abstract

Astronomical Journal, vol. 84, Jan. 1979, p. 50-55.

Mathematics

5

Frequency Distribution, Galactic Clusters, Many Body Problem, Computerized Simulation, Gravitational Effects, Harmonics, Vectors (Mathematics), Virial Theorem

Scientific paper

The set of separation vectors for three N-body simulations provided by Wielen (1974) is used to derive the mean radii, mean harmonic radii, clumpiness parameters, and concentration indexes as a function of mass sample and of time for each model. Frequency distributions of the separation vectors are also presented for each model as a function of mass sample and of time. These data are compared with the data for observed clusters provided by Hickson (1977). Close parallels between the model data and the data for observed clusters are discussed, including the time development of structure in the frequency distributions of separations.

Affiliated with

Also associated with

No associations

Rating

Clusters of galaxies compared with N-body simulations - The set of separation vectors 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 Clusters of galaxies compared with N-body simulations - The set of separation vectors, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clusters of galaxies compared with N-body simulations - The set of separation vectors will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1141032