报告人：王有刚　副研究员  （国家天文台）

时间：2015年12月9日下午4：00

地点：东区理化大楼18层天文台报告厅

报告摘要：Our own Milky Way is the nearest barred galaxy. Compared with other distant galaxies, the Galaxy extensive observed photometric and kinematic data which enable us to study the bar structure in detail. A though understanding of the structure and dynamics of the Galactic bar may help us understand the formation of other spiral galaxies,  and test the validity of the popular cold dark matter structure formation model. In this talk, I will report our recent studies on the dynamical model of the Milky Way bar by using the Schwarzschild's orbit-superposition and Made-to-Measure methods. In the end of the talk, I will briefly report on the on-going project, constructing the Milky Way dynamical model by using the LAMOST data.