
研究机构: 物理与天文学院
研究领域: 宇宙学和宇宙大尺度结构 天文学数值模拟 星系群和星系团 星系形成和演化
办公电话: 021-54740008
电子邮箱: xyang@sjtu.edu.cn
1.Yang,X., Zhang, Y., Lu, T., Wang, H., Shi, F., Tweed, D., Li, S., Luo, W., Lu, Y., Yang, L.,2017., Revealing the cosmic web dependent halo bias. ArXiv e-prints arXiv:1704.02451.
2.Yang, X., Mo, H.~J., van den Bosch, F.~C., Bonaca, A., Li, S., Lu, Y., Lu, Y., Lu, Z.,2013.,Constraining the Star Formation Histories in Dark Matter Halos. I. Central Galaxies.,The Astrophysical Journal 770, 115
3.Yang, X., Mo, H. J., van den Bosch, F. C., Zhang, Y., Han, J. 2012. Evolution of the Galaxy-Dark Matter Connection and the Assembly of Galaxies in Dark Matter Halos. ApJ, 752, 41.
4.Yang, X., Mo, H. J., Zhang, Y., van den Bosch, F. C. 2011. An Analytical Model for the Accretion of Dark Matter Subhalos. ApJ, 741, 13.
5.Liu, L., Yang X., Mo, H. J., van den Bosch, F. C., Springel, V. 2010.The Stellar Mass Components of Galaxies: Comparing Semi-Analytical Models with Observation. ApJ, 712, 734-745.
6.Yang, X., H.J.Mo, and F.C.van den Bosch, (2009), Galaxy Groups in the SDSS DR4. III. The Luminosity and Stellar Mass Functions. ApJ, 695, 900-916 .
7.Yang, X., H.J.Mo, and F.C.van den Bosch, (2009), The Subhalo-Satellite Connection and the Fate of Disrupted Satellite Galaxies. ApJ, 693, 830-838
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