报告摘要：Dwarf galaxy integral survey is a program to obtain 3-D spectra of a volume/flux-limited sample of local dwarfs within 11 Mpc, along with a complementary sample of some exceptional dwarfs such as ultra diffuse galaxies. In this talk, I would like to give some early results from this survey including dark matter distribution, intermediate-massive black holes and interstellar media in dwarfs.
主讲人简介：Yong Shi received his Ph.D in astronomy in 2008 from the Department of Astronomy at the University of Arizona. He spent about four years in California Institute of Technology as post-doc, and then joined the faculty of Nanjing University in 2013. His main research area is galaxy formation and evolution through observations.
