报告题目:New views on the Andromeda galaxy M31
报 告 人:David Valls-Gabaud (Observatoire de Paris, CNRS, IHEP, NAOC)
报告摘要:The detailed analysis of colour-magnitude diagrams obtained at the Canada-France-Hawaii telescope has revealed hitherto unknown properties of the nearest spiral galaxy, M31. The recent star formation history in the disc shows that M31 is a starving galaxy in the so-called green valley. Time-domain series carried out over two years provide the first comprehensive variability inventory of this galaxy. Hubble Space Telescope follow-up observations of some of the Cepheids discovered have led to a determination of its distance with an error of 3%, and likewise for the Hubble constant, by-passing the uncertainties in the calibration of the Magellanic Clouds. The analysis of the halo fields has revealed not only many substructures at faint surface brightness levels, but a wealth of information on new satellites, globular clusters, stellar streams, and the structure of the halo. Over half of the satellites of M31 appear to lie in a vast disc, which is rotating around the galaxy, yielding stringent constraints on the accretion mechanisms which lead to the formation of galaxies.
时 间:2014年3月5日周三 上午10:00
地 点:紫台大楼619会议室
联 系 人:李月月(83332162)
欢迎大家积极参加!
紫金山天文台学术委员会学术交流工作委员会