SCALING ANALYSIS OF THE GALAXY DISTRIBUTION IN THE SSRS CATALOG

被引：4

作者：

CAMPOS, A ^{[1
]}

DOMINGUEZTENREIRO, R ^{[1
]}

YEPES, G ^{[1
]}

机构：

[1] UNIV AUTONOMA MADRID,DEPT FIS TEOR 111,E-28049 CANTO BLANCO,SPAIN

来源：

ASTROPHYSICAL JOURNAL | 1994年 / 436卷 / 02期

关键词：

GALAXIES; CLUSTERING; FUNDAMENTAL PARAMETERS;

D O I：

10.1086/174931

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A detailed analysis of the galaxy distribution in the Southern Sky Redshift Survey (SSRS) by means of the multifractal or scaling formalism is presented. It is shown that galaxies duster in different ways according to their morphological type as well as their size. Elliptical galaxies are more clustered than spirals, even at scales up to 15 h(-1) Mpc, whereas no clear segregation between early and late spirals is found. It is also shown that smaller galaxies distribute more homogeneously than larger galaxies.

引用

页码：565 / 575

页数：11

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