How to measure star formation rates in galaxies?

被引：0
|
作者：
Buat, Veronique [1 ]
机构：
[1] Aix Marseille Univ, CNRS, LAM, UMR7326, F-13388 Marseille, France
来源：
INTRODUCTION TO COSMOLOGY | 2016年 / 2卷
关键词：
STELLAR POPULATION PROPERTIES; DUST ATTENUATION; FORMING GALAXIES; FORMATION HISTORY; NEARBY GALAXIES; MAIN-SEQUENCE; H-ALPHA; ULTRAVIOLET; UNIVERSE; FLUXES;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Our knowledge of cosmic mass assembly deeply relies on measurements of star formation rates as a function of redshift. This parameter must be estimated in a consistent manner, with a good knowledge of systematics, before studying its correlation with other quantities such as stellar or gas masses. Constraining the rate at which galaxies form stars across the Universe is of utmost importance if we want to understand galaxy formation and evolution.
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收藏
页码：134 / 141
页数：8
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