“About Me”的版本间的差异
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*The size distruibution of galaxies [http://adsabs.harvard.edu/abs/2003MNRAS.343..978S] | *The size distruibution of galaxies [http://adsabs.harvard.edu/abs/2003MNRAS.343..978S] | ||
*The Tully-Fisher relation of Spiral galaxies | *The Tully-Fisher relation of Spiral galaxies | ||
:The third parameter, fundamental plane? | :The third parameter, fundamental plane?[http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] | ||
:Morphological dependence? | :Morphological dependence?[http://adsabs.harvard.edu/abs/2009ApJ...705.1496S] | ||
*The inclination of spiral galaxies | *The inclination of spiral galaxies | ||
:inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies. | :inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies.[http://adsabs.harvard.edu/abs/2007ApJ...659.1159S] | ||
:inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs. | :inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs.[http://adsabs.harvard.edu/abs/2010ApJ...725L.210S] | ||
===X-ray Astronomy=== | ===X-ray Astronomy=== | ||
2014年9月9日 (二) 14:05的版本
Prof. Dr. Shiyin Shen
- Vice director of the Research Center of the Galaxy and Cosmology ;
- Deputy leader of the research group Star cluster and Galactic Structure;
Research Fields
galaxy astronomy
- statistical porperties of galaxies and AGNs
X-ray astronomy
- image stacking technic; QSO, clusters of galaxies
LAMOST extragalactic survey
- Suvey Strategy, input source catalog
- South galactic Cap U-band Sky Suvey ([1])
Research highlights
Statsitical properties of galaxies
- The statistical nature of the brightest group galaxies [2]
- The size distruibution of galaxies [3]
- The Tully-Fisher relation of Spiral galaxies
- The inclination of spiral galaxies
- inclination dependence luminosity function of spiral galaxies: implications on the dust attenuation of galaxies.[6]
- inclination of the host spirals of type II AGNs: implications on the nuclear obscurer of the AGNs.[7]
X-ray Astronomy
- Soft X-ray properties of QSOs
- X-ray properties of clusters of galaxies