Cold gas contents of galaxies and their relations to the stellar and dark-matter components  

作　　者：Houjun Mo 

机构地区：[1]Department of Astronomy,University of Massachusetts,Amherst MA 01003,USA

出　　处：《Science China(Physics,Mechanics & Astronomy)》2024年第11期180-180,共1页中国科学：物理学、力学、天文学（英文版）

摘　　要：One of the most important goals of modern cosmology is to understand how galaxies form and evolve in ecosystems defined by the cosmic density field. The formation of galaxies is a process through which cold baryonic gas, dominated by neutral hydrogen(HI), is converted into stars.

关 键 词：GALAXIES STELLAR STARS 

分 类 号：P144[天文地球—天体物理]