14/10/27-14/10/31

 

SHAO Astrophysics Colloquia 

Title: What do we really know about DM?

Speaker: 陶嘉琳 (教授，清华大学)

Time: Thursday, 3:00pm, October 30th

Location: Lecture Hall, 3rd floor  

Abstract: Evidence for DM comes from a wealth of astrophysical observations that I will briefly review in this talk, with an emphasis on the problems we still wish to solve.

 

Seminar talk

 

Title: Millimeter/submillimeter follow-up of Herschel high-z galaxies.  

         H2O, a new diagnosis of their dense cores  

Speaker: Alain Omont (IAP)  

Time: Wednesday, 3:00pm, Oct 29  

Location: the middle conference room

   

Group meetings and additional talks

 

Observational High Energy Astrophysics Group Seminar  

Location: 1401; Contact: Zhen Yan <zyan@shao.ac.cn>  

• Very late photometry of SN 2011fe  (Dongming Mao)  
• Discovery of a correlation between the frequency of the mHz quasi-periodic oscillations and the neutron-star temperature in the low-mass X-ray binary 4U 1636–53 (Holger Stiele)  
• X-Raying an Accretion Disk in Realtime_the Evolution of Ionized Reflection during a Superburst from 4U 1636-536 (Wenda Zhang)  
• An ultraluminous X-ray source powered by an accreting neutron star (Zhen Yan)  

Time: Monday, 10:30am, Oct 27  

   

Blackhole accretion and High-energy astrophysics Seminar  

Location: 1608; Contact: Qixiang Yang <qxyang@shao.ac.cn>

Title: AGN Type-casting: Mrk 590 No Longer Fits the Role  

Speaker: Fu-Guo Xie  

Time: Tuesday, 2:00 pm, Oct 28