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2022_autumn
2022-08-22
沈世银
星系光谱(不包含发射线)中的熵(信息量)的最小的特征就是D4000和Hdelta arXiv:2208.05489
IFS观测中气相金属丰度的两点相关的测量及模型解释:相关长度,注入半径 arXiv:2206.08072
星系中星族的恒星金属丰度与引力势(M/R)有一个较为紧密而且红蓝星系相互统一的关系 arXiv:2208.06939
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