银河恒星形成的解剖:不同模式的气体吸积、反馈和再循环的角色

M. Noguchi
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引用次数: 0

摘要

冷模式气体吸积与热模式气体吸积的同时存在,可以解释星系恒星形成历史在星系质量上的多样性。我们研究了各种物理过程在产生观察到的多样性中的作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Anatomy of Galactic Star Formation: Roles of Different Modes of Gas Accretion, Feedback, and Recycling
Abstract Existence of the cold-mode gas accretion along with the hot-mode accretion can explain the diversity in the galactic star formation history across galaxy mass. We examine the role of various physical processes in producing the observed diversity.
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