The local space density of dwarf galaxies

被引:51
作者
Loveday, J
机构
[1] Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637
关键词
cosmology; observations; galaxies; distances and redshifts; evolution; luminosity function; mass function; surveys;
D O I
10.1086/304778
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We estimate the luminosity function of field galaxies over a range of 10 mag (-22 < M-BJ < -12 for H-0 = 100 km s(-1) Mpc(-1)) by counting the number of faint APM galaxies around Stromlo-APM redshift survey galaxies at known distance. The faint end of the luminosity function rises steeply at M-BJ approximate to -15, implying that the space density of dwarf galaxies is at least 2 times larger than predicted by a Schechter function with flat faint-end slope. Such a high abundance of dwarf galaxies at low redshift can help explain the observed number counts and redshift distributions of faint galaxies without invoking exotic models for galaxy evolution.
引用
收藏
页码:29 / 36
页数:8
相关论文
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