U-band luminosity dependence of galaxy clustering in the main galaxy sample of SDSS DR10

被引：0

作者：

Zhang, Fuyang ^{[1
]}

Deng, Xin-Fa ^{[2
]}

机构：

[1] Nanchang Univ, Sch Informat Engn, Nanchang 330031, Jiangxi, Peoples R China

[2] Nanchang Univ, Sch Sci, Nanchang 330031, Jiangxi, Peoples R China

来源：

ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2014年 / 40卷 / 12期

基金：

美国国家科学基金会;

关键词：

galaxy; fundamental parameters-galaxy; large scale structure; DIGITAL SKY SURVEY; 2DF REDSHIFT SURVEY; STAR-FORMATION RATE; ENVIRONMENTAL DEPENDENCE; DATA RELEASE; OPTICAL-PROPERTIES; SUPERCLUSTERS; COLOR; MORPHOLOGY; FILAMENTS;

D O I：

10.1134/S1063773714120081

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using two volume-limited Main galaxy samples of the Sloan Digital Sky Survey Data Release 10 (SDSS DR10), we study u-band luminosity dependence of galaxy clustering by cluster analysis. Statistical results of two volume-limited Main galaxy samples are the same: luminous galaxies in M (u) preferentially form isolated galaxies, close pairs and small groups at all scales, whereas faint galaxies in M (u) preferentially inhabit dense groups and clusters.

引用

页码：753 / 758

页数：6

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