Home | Contact | Sitemap | 中文 | CAS
Search:
About Us Research People International Cooperation News Education & Training Join Us Journals Papers Resources Links
Location: Home > News > Seminars
News
  • Events
  • DAMPE
  • Seminars
  • Research Trends
  • Star Formation in the Extended Disks of Spiral Galaxies and what it tells us about the Disk Mass Distribution

    Seminar Title  

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

       
    Speaker:   Dr. Mousumi Das
       

     Affiliation:    

    (Associate ProfessorI, Indian Institute of Astrophysics)  

       
    When Monday morning, Sep. 4, 10:30 a.m
       

    Where:   

    Room 619, Office Block, 2 West Beijing Road (PMO, CAS)
     

                             Welcome to Attend   

     
      ( PMO Academic Committee & Academic Circulating committee)
     

       Abstract: 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.

    Copyright © Purple Mountain Observatory, CAS,2 West Beijing Road, Nanjing 210008, China
    Phone: 0086 25 8333 2000 Fax: 8333 2091 http://english.pmo.cas.cn