CLUSTERING OF GALAXIES BY INVERSE CASCADE IN A TURBULENT MEDIUM

被引：11

作者：

KRISHAN, V

SIVARAM, C

机构：

[1] Indian Institute of Astrophysics, Bangalore

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1991年 / 250卷 / 01期

关键词：

D O I：

10.1093/mnras/250.1.157

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Non-linear interactions between small fluid elements in an energetically open non-linear system facilitate the formation of large coherent stable structures. This is known as self-organization. We interpret the clustering of galaxies on all scales as the result of self-organization processes occurring in a turbulent medium.

引用

页码：157 / 160

页数：4

共 21 条

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BURSTEIN D, 1986, GALAXY DISTANCES DEV, P123

[2] MAGNETIC-FIELDS IN THE EARLY UNIVERSE [J].