In order to explain observedAMR and its scatter, mechanisms of diffusion of stellar orbitsand non-instantaneous mixing must be considered in Galacticchemical evolution models.

 
  • 为了解释观测的年龄--金属丰度关系及其弥散,银河系化学演化模型必须考虑恒星轨道运动、非瞬时混合等机制。
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