Image Details
Caption: Fig. 1.
Evolution of the abundance of clusters with redshift z for three distinct cosmologies. Only clusters with mass ﹩M\geq 8\times 10^{14}\,h^{-1}\,M_{\odot }﹩ within their virial radius ﹩R_{\mathrm{vir}\,}﹩ are considered. The solid curve represents an open universe (﹩\Omega _{0}=0.3,\Omega _{\Lambda }=0﹩), the dashed curve a flat universe (﹩\Omega _{0}=0.3,\Omega _{\Lambda }=0.7﹩), and the dotted curve a closed universe (﹩\Omega _{0}=1.0,\Omega _{\Lambda }=0﹩).
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.