In this review I demonstrate that a realistic model for the formation of galaxy disks depends on a proper treatment of the gas in galaxies. Historically. cosmological simulations of disk galaxy formation have suffered from a lack of resolution and a physically motivated feedback prescription. Recent computational progress has allowed for unprecedented resolution, which in turn allows for a more realistic treatment of feedback. These advances have led to a new examination of gas accretion, evolution, and loss in the formation of galaxy disks. Here I highlight the role that gas inflows, the regulation of gas by feedback, and gas outflows play in achieving simulated disk gala xies that better match observational results as a function of redshift.
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机译:通过使用包括版本信息的控制信息来存储信息的方法信息的存储方法用于记录和/或再现到记录和/或再现的设备关于具有控制信息的信息的数据存储磁盘上的数据。现有信息和控制信息已更新。信息存储的M ecvel用于通过读取单元进行记录/回放/根据数据的再现磁盘的信息。用于记录和/或再现的设备,用于记录和/或再现数据。根据从磁盘读取的信息,用于存储信息的数据传输方法,用于检测信息的存储。 m u00ecdia通过 u00ecvel在计算机中阅读。