“About Me”的版本间的差异
跳到导航
跳到搜索
| （未显示同一用户的1个中间版本） | |||
| 第6行： | 第6行： | ||
* galaxy structure, dust geometry of MW and local disk galaxies [http://adsabs.harvard.edu/abs/2017AJ....153...88L][http://adsabs.harvard.edu/abs/2018ApJ...858...75L] | * galaxy structure, dust geometry of MW and local disk galaxies [http://adsabs.harvard.edu/abs/2017AJ....153...88L][http://adsabs.harvard.edu/abs/2018ApJ...858...75L] | ||
* galaxy pair and galaxy interaction [https://ui.adsabs.harvard.edu/abs/2016RAA....16...43S/abstract] [https://ui.adsabs.harvard.edu/#abs/2019ApJ...880..114F/abstract] [https://ui.adsabs.harvard.edu/abs/2020ApJS..246...12Z/abstract] | * galaxy pair and galaxy interaction [https://ui.adsabs.harvard.edu/abs/2016RAA....16...43S/abstract] [https://ui.adsabs.harvard.edu/#abs/2019ApJ...880..114F/abstract] [https://ui.adsabs.harvard.edu/abs/2020ApJS..246...12Z/abstract] | ||
* IFS study of galaxies [https://ui.adsabs.harvard.edu/abs/2018A%26A...613A..13Y/abstract] [https://ui.adsabs.harvard.edu/#abs/2020ApJ...892L..20F/abstract] | |||
* statistical applications on large sample of galaxies and AGNs [http://adsabs.harvard.edu/abs/2006MNRAS.369.1639S] [http://adsabs.harvard.edu/abs/2014ApJ...782...23S][] | * statistical applications on large sample of galaxies and AGNs [http://adsabs.harvard.edu/abs/2006MNRAS.369.1639S] [http://adsabs.harvard.edu/abs/2014ApJ...782...23S][] | ||
* scaling relation of disk galaxies [http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] [http://adsabs.harvard.edu/abs/2009ApJ...705.1496S] | * scaling relation of disk galaxies [http://adsabs.harvard.edu/abs/2002MNRAS.331..259S] [http://adsabs.harvard.edu/abs/2009ApJ...705.1496S] | ||
| 第16行： | 第16行： | ||
* 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] | ||
* 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] | ||
==Curriculum Vitae 个人简历 == | ==Curriculum Vitae 个人简历 == | ||
2020年4月29日 (三) 14:52的最新版本
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]
- IFS study of galaxies [6] [7]
- statistical applications on large sample of galaxies and AGNs [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]