2013/12/4

From cluster group wiki

Revision as of 06:14, 13 December 2013 by Cluster (talk | contribs)

(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)

Jump to navigation Jump to search

沈世银 EG sources in LAMOST DR1

甘建铃LAMOST的球状星团的金属丰度的测量问题

可以利用FSPS的code

钟靖 LAMOST光谱的IDL可视化程序

常瑞香: 银河系结构模型, Du et al. 2006
李静 M巨星在WISE里面的颜色

WISE的W1-W4能很好的区分巨星和矮星

Retrieved from "http://cluster.shao.ac.cn/wiki/index.php?title=2013/12/4&oldid=186"