COMPARATIVE STUDIES OF CLUSTERING PROPERTIES BETWEEN PASSIVE GALAXIES AND STAR-FORMING ONES

被引：11
作者：
Deng, Xin-Fa [1 ]
He, Ji-Zhou [1 ]
Chen, Yi-Qing [1 ]
Song, Jun [1 ]
Jiang, Peng [1 ]
机构：
[1] Nanchang Univ, Sch Sci, Nanchang 330031, Jiangxi, Peoples R China
来源：
ASTROPHYSICAL JOURNAL | 2009年 / 706卷 / 01期
基金：
中国国家自然科学基金; 美国国家航空航天局; 美国国家科学基金会;
关键词：
galaxies: fundamental parameters; large-scale structure of universe; DIGITAL SKY SURVEY; SPECTROSCOPIC TARGET SELECTION; 2DF REDSHIFT SURVEY; DATA RELEASE; FORMATION RATES; LUMINOSITY DEPENDENCE; INTERACTING GALAXIES; SPIRAL GALAXIES; SPECTRAL TYPE; COLOR;
D O I：
10.1088/0004-637X/706/1/436
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Using the volume-limited Main galaxy sample of the Sloan Digital Sky Survey Data Release 6, we have explored the dependence of clustering properties of galaxies on the star formation activity. It is found that star-forming galaxies preferentially form isolated, close double and multiple systems, while passive galaxies preferentially inhabit the dense groups and clusters. We also construct the two samples with the same galaxy number and number density, and reach the same conclusion, which shows that our statistical conclusion is robust.
引用
收藏
页码：436 / 440
页数：5
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