The morphological dependent Tully-Fisher relation of spiral galaxies (2009)
Shen, Shiyin, Wang, Caihong, Chang, Ruixiang, Shao, Zhengyi, Hou, Jinliang, Shu, Chenggang
The Tully-Fisher relation of spiral galaxies shows notable dependence on morphological types, with earlier type spirals having systematically lower luminosity at fixed maximum rotation velocity...
Comparisons between isothermal and NFW mass profiles for strong-lensing galaxy clusters (2008)
Shu, Chenggang, Zhou, Binglu, Bartelmann, Matthias, Comerford, Julia M., Mellier, Yannick
While both isothermal and NFW-based mass models for galaxy clusters are widely adopted in strong-lensing studies, they cannot easily be distinguished based solely on observed positions of arcs and...
Color-magnitude relations of late-type galaxies (2006)
Chang, Ruixiang, Shen, Shiyin, Hou, Jinliang, Shu, Chenggang, Shao, Zhengyi
We use a large sample of galaxies drawn from the Sloan Digital Sky Survey (SDSS) and Two Micro All Sky Survey (2MASS) to present Color-Magnitude Relations (CMRs) for late-type galaxies in both...
An analytic model for the galactic winds and mass outflows (2003)
Shu, Chenggang, Mo, H. J., Mao, Shude
Galactic winds and mass outflows are observed both in nearby starburst galaxies and in high-redshift star-forming galaxies. In this paper we develop a simple analytic model to understand the observed...
The Fundamental Plane of Spiral Galaxies: Theoretical Expectations (2001)
Shen, Shiyin, Mo, H. J., Shu, Chenggang
Current theory of disk galaxy formation is used to study fundamental-plane (FP) type of relations for disk galaxies. We examine how the changes in model parameters affect these relations and explore...
The Host Haloes of Lyman Break Galaxies and Sub-millimeter Sources (2001)
Shu, Chenggang, Mao, Shude, Mo, H. J.
We use the observed sizes and star formation rates of Lyman-break galaxies (LBGs) to understand their properties expected in the hierarchical scenario of galaxy formation. The observed size...
Some statistical properties of spiral galaxies (2000)
Ma, Jun, Zhao, Junliang, Shu, Chenggang, Peng, Qiuhe
This paper presents some statistical correlations of 72 northern spiral galaxies. The results show that early-type spirals that are brighter, and thicker, and the axis ratios ($H_{z}/H_r$) of the...
Dependence of Spiral Galaxy Distribution on Viewing Angle in RC3 (2000)
Ma, Jun, Song, Guoxuan, Shu, Chenggang
The normalized inclination distributions are presented for the spiral galaxies in RC3. The results show that, except for the bin of $81^{\circ}$-$90^{\circ}$, in which the apparent minor isophotal...
Star Formation and Chemical Evolution of Lyman-Break Galaxies (2000)
The number density and clustering properties of Lyman-break galaxies (LBGs) observed at redshift $z\sim 3$ are best explained by assuming that they are associated with the most massive haloes at...