天文学进展2016，Vol.34Issue(4)：477-485,9.DOI:10.3969/j.issn.1000-8349.2016.04.09
恒星形成的辐射流体（磁流体）数值模拟研究进展
Research Progress in Numerical Simulation Study of Star Formation Based on Radiation Hydrodynamics (Magnetohydrodynamics)
摘要
Abstract
Stars are one of the most important objects in the universe and study of star formation is an important research subject. Astronomers are trying to understand a series of problems associated with star formation, which include how massive stars and star cluster form, what processes determines the physical properties of star-forming region, what deter-mines the initial mass function, what determines the star formation rate, and so on. Recently, numerical simulations of star formation continues to make progress. This paper focuses on research progress in the numerical study of protostellar collapse, massive star formation, frag-mentation and collapse of molecular cloud, star cluster formation and the initial mass function, based on radiation hydrodynamics (magnetohydrodynamics).关键词
恒星形成/辐射转移/数值模拟Key words
star formation/radiative transfer/numerical simulation分类
天文与地球科学引用本文复制引用
杨孝鸿..恒星形成的辐射流体（磁流体）数值模拟研究进展[J].天文学进展,2016,34(4):477-485,9.基金项目
中央高校基本科研业务(106112016CDJXY300007)；国家自然科学基金(11547305) （106112016CDJXY300007）
