THE MASS FUNCTION OF NEARBY GALAXY CLUSTERS

被引：32
|
作者：
BIVIANO, A
GIRARDI, M
GIURICIN, G
MARDIROSSIAN, F
MEZZETTI, M
机构：
[1] INST ASTROPHYS,F-75014 PARIS,FRANCE
[2] UNIV TRIESTE,DIPARTIMENTO ASTRON,I-34100 TRIESTE,ITALY
来源：
ASTROPHYSICAL JOURNAL | 1993年 / 411卷 / 01期
关键词：
GALAXIES; CLUSTERING;
D O I：
10.1086/186900
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present the distribution of virial masses for nearby galaxy clusters, as obtained from a data set of 75 clusters, each having at least 20 galaxy members with measured redshifts within 1.5 h-1 Mpc. After having accounted for problems of incompleteness of the data set, we fitted a power law to the cluster mass distribution.
引用
收藏
页码：L13 / L16
页数：4
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