Statistics – Computation
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mnras.248..332b&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 248, Jan. 15, 1991, p. 332-352.
Statistics
Computation
333
Computational Astrophysics, Galactic Clusters, Galactic Evolution, Self Consistent Fields, Astronomical Models, Many Body Problem, Red Shift
Scientific paper
The original Press-Schechter (1974) theory is extended to provide a mathematical description of the evolution of a subset of regions that will eventually collapse to form clusters of a set mass. The conditional multiplicity function of groups at an epoch with redshift z is obtained and is combined with the present distribution of group masses in order to obtain the joint multiplicity function. These multiplicity functions are used to study the evolutionary histories of groups and clusters.
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