“About Me”的版本间差异
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无编辑摘要 |
无编辑摘要 |
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* Are the brightest group/cluster galaxies special? Is it only because of their definition? [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] |
* Are the brightest group/cluster galaxies special? Is it only because of their definition? [http://adsabs.harvard.edu/abs/2014ApJ...782...23S] |
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* The size distribution (size-mass relation) of local galaxies [https://ui.adsabs.harvard.edu/abs/2003MNRAS.343..978S/abstract] |
* The size distribution (size-mass relation) of local galaxies [https://ui.adsabs.harvard.edu/abs/2003MNRAS.343..978S/abstract] |
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==Curriculum Vitae 个人简历 == |
==Curriculum Vitae 个人简历 == |
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2020年4月29日 (三) 14:30的版本
Prof. Dr. Shiyin Shen
- orcid: 0000-0002-3073-5871
- Deputy leader of the research group Star cluster and Galaxies;
Research Interests
- galaxy structure, dust geometry of MW and local disk galaxies [1][2]
- galaxy pair and galaxy interaction [3] [4] [5]
- statistical applications on large sample of galaxies and AGNs [6] [7][]
- IFS study of galaxies [8] [9]
- scaling relation of disk galaxies [10] [11]
Research highlights
- How to model the three-dimensional dust distribution of MW? What is the vertical distance of the Sun to the Galactic plane? [12]
- LAMOST Complementary galaxy sample: these galaxies in SDSS main galaxy sample without spectroscopy [13]
- Whether the universe is transparent? [14]
- Are the brightest group/cluster galaxies special? Is it only because of their definition? [15]
- The size distribution (size-mass relation) of local galaxies [16]