SSRS目录中银河分布的比例分析
天体物理学
2009-10-22 v1
摘要
presented 对南天红移调查(SSRS)中银河分布的详细分析，采用多ficntl或比例形式化方法。结果表明，根据星系的形态类型及其大小，银河的聚集方式不同。椭圆星系的聚集程度高于旋星系，即使在15 h Mpc的尺度上也是如此，而且在早期和晚期旋星系之间找不到明确的区分。还表明，较小的星系比较大的星系更均匀地分布。
引用
@article{arxiv.astro-ph/9407041,
title = {Scaling Analysis of the Galaxy Distribution in the SSRS Catalog},
author = {A. Campos and R. Dominguez-Tenreiro and G. Yepes},
journal= {arXiv preprint arXiv:astro-ph/9407041},
year = {2009}
}
备注
12 pages uuencoded compressed Postscript file with figures included (380 K). To appear in ApJ, December 1994. Also available by anonymous ftp from dust0.dur.ac.uk in /pub/preprints/campos_ssrs.ps