内网平台 网站地图 联系我们 English 中国科学院
首页紫台简介机构设置新闻动态科研成果研究队伍合作交流天文学院创新文化党群园地信息公开
新闻动态
图片新闻
综合新闻
天文快讯
Colloquium & 学术交流
国内外天文学术会议
紫台通讯
传媒扫描
科普动态
科研信息
台内新闻
您当前的位置:首页>新闻动态>Colloquium & 学术交流
9月4日 Star Formation in the Extended Disks of Spiral Galaxies and what it tells us about the Disk Mass Distribution
2017年08月28日

  题目: Star Formation in the Extended Disks of Spiral Galaxies and what it tells us about the Disk Mass Distribution

  报告人:Mousumi Das (Associate ProfessorI, Indian Institute of Astrophysics)

  摘要:A large fraction of spiral galaxies show filamentary or diffuse star formation well beyond their optical disks, in regions where the disk surface density lies below the threshold for star formation. Cold gas accretion onto the outer disks is thought to drive this star formation. The nature of star formation in such adverse environments where the dark matter halo dominates the mass content, is not well understood. In this talk I will first present some preliminary UV observations of extended disk star formation done with the Ultraviolet Imaging Telescope (UVIT) in two galaxies. Using observations and modelling of another galaxy NGC4701, I discuss how the disk dark matter also plays a role in supporting the extended disk star formation in galaxies. We also briefly describe how this phenomenon can be used to trace dark matter in our low redshift Universe.

  报告时间:2017年9月4日,星期一,上午10:30

  报告地点:紫台办公大楼 619 会议室

欢迎大家参加!

                                                    紫金山天文台学术委员会

地址:(210033)江苏省南京市栖霞区元化路10号  电话:86-25-83332000  传真:86-25-83332091
版权所有:中国科学院紫金山天文台 http://www.pmo.cas.cn pmoo@pmo.ac.cn 备案序号:苏ICP备05007736号