Luminosity and clustering of galaxies selected by EW(Halpha)
msra(1999)
摘要
We study the luminosity function and clustering properties of subsamples of
local galaxies selected from the Stromlo-APM survey by the rest-frame
equivalent width (EW) of the Halpha emission line. The b_J luminosity function
of star-forming galaxies has a significantly steeper faint-end slope than that
for quiescent galaxies: the majority of sub-L* galaxies are currently
undergoing significant star formation. Emission line galaxies are less strongly
clustered, both amongst themselves, and with the general galaxy population,
than quiescent galaxies. Thus as well as being less luminous, star-forming
galaxies also inhabit lower-density regions of the Universe than quiescent
galaxies.
更多查看译文
关键词
star formation,cluster of galaxies,equivalent width,luminosity function,emission line
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要