COMPARISON OF LIKELY CANDIDATE MODELS FOR ABELL CLUSTER STRUCTURES AGAINST THE OBSERVED DISTRIBUTION

被引：1

作者：

BATUSKI, DJ

MELOTT, AL

SCHERRER, RJ

BERTSCHINGER, E

机构：

[1] UNIV KANSAS,DEPT PHYS & ASTRON,LAWRENCE,KS 66045

[2] OHIO STATE UNIV,DEPT PHYS,COLUMBUS,OH 43210

[3] MIT,DEPT PHYS,CAMBRIDGE,MA 02139

来源：

ASTROPHYSICAL JOURNAL | 1991年 / 367卷 / 02期

关键词：

COSMOLOGY; GALAXIES; CLUSTERING;

D O I：

10.1086/169637

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The amount of structure in the Abell cluster distribution is compared with a variety of "likely candidate" models, including a minimal isocurvature baryon model, a low-density universe model with baryons and cosmic strings, and a model with hot dark matter and cosmic strings. The hot dark matter and cosmic string model does best at reproducing the characteristics of the observed data sample.

引用

页码：393 / 398

页数：6

共 24 条

[1]

Abell G. O., 1958, ASTROPHYS J SUPPL S, V3, P211

[2]

BAHCALL NA, 1988, ANNU REV ASTRON ASTR, V26, P631

[3] A SUPERCLUSTER CATALOG [J].