“2013 publications”的版本间差异
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*Using L dwarfs with distances to test models[http://adsabs.harvard.edu/abs/2013IAUS..289..425W] |
*Using L dwarfs with distances to test models[http://adsabs.harvard.edu/abs/2013IAUS..289..425W] |
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:Wang, Youfen; Jones, H. R. A.; Smart, R. L.; Shao, Z., 2013IAUS..289..425W |
:Wang, Youfen; Jones, H. R. A.; Smart, R. L.; Shao, Z., 2013IAUS..289..425W |
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*一种新的疏散星团成员判定方法[http://d.g.wanfangdata.com.cn/Periodical_twxb201305005.aspx] |
*一种新的疏散星团成员判定方法[http://d.g.wanfangdata.com.cn/Periodical_twxb201305005.aspx] |
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:Hu, Tao; Shao, Zhengyi; Peng, Qiuhe, 2013ApJ...762L..27H |
:Hu, Tao; Shao, Zhengyi; Peng, Qiuhe, 2013ApJ...762L..27H |
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*Disk thickness and spiral arm structure of M31[http://adsabs.harvard.edu/abs/2013NewA...23...49H] |
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:Hu, Tao; Shao, Zhengyi; Wang, Min; Peng, Qiuhe, 2013NewA...23...49H |
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2014年10月21日 (二) 02:22的最新版本
First Author
- Star formation and metallicity gradients in semi-analytic models of disc galaxy formation[1]
- Fu et al. 2013MNRAS.434.1531F
- The roles of atomic and molecular gas on the redshift evolution of star formation and metallicity in galaxy formation models[2]
- Fu, Jian; Kauffmann, Guinevere 2013IAUS..292..245F
- Using L dwarfs with distances to test models[3]
- Wang, Youfen; Jones, H. R. A.; Smart, R. L.; Shao, Z., 2013IAUS..289..425W
- 一种新的疏散星团成员判定方法[4]
- 高新华，陈力，侯振杰，2013，天文学报，54,439
- 银盘径向丰度梯度及冷气体的演化
- 陈麒似，常瑞香，尹君. 2013，天文学报
Coauthors
- New Estimates of the Inclination, Position Angle, Pitch Angle, and Scale Height of the Whirlpool Galaxy[5]
- Hu, Tao; Shao, Zhengyi; Peng, Qiuhe, 2013ApJ...762L..27H
- Disk thickness and spiral arm structure of M31[6]
- Hu, Tao; Shao, Zhengyi; Wang, Min; Peng, Qiuhe, 2013NewA...23...49H
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