The stellar population membership of each star is determined by the pure kinematics criterions. Lastly, we discussed the photometric age-metallicity relation of thin and thick disk stars.
然后用纯运动学标准确定了样本A和B中每颗恒星的星族成分,分别讨论了薄盘和厚盘恒星测光的年龄-金属丰度关系。
参考来源 - 不同星族恒星的年龄—金属丰度关系·2,447,543篇论文数据,部分数据来源于NoteExpress
应用推荐