USTC Astronomy Colloquium Series: 2019 Spring
The Milky Way satellite galaxies
康熙 研究员
紫金山天文台
2019/04/30, 4:00pm , the 19th-floor Observatory Hall
Our Milky Way is an ideal local laboratory to test the standard cosmology and galaxy formation physics. The satellite galaxies of MW display unusual distribution in their spatial and kinematical properties. In this talk I will introduce the recent progress on three main problems of MW satellites: Great plane, missing satellite and too-big-to-fail. I will also present an analytical model to study the evolution of MW satellites.
Xi Kang is a research scientist at PMO. He got his PhD at Shanghai Astronomical Observatory in 2005, and then did his postdoc at the University of Oxford and Max-Planck-Institute for Astronomy. He joined PMO in 2009, leading an independent research group on galaxy and cosmology. His main research interests focus on theoretical modeling of galaxy formation, large-scale structure and N-body simulations.