SHAO Astrophysics Colloquia  

　　    

The Evolution of the Main Sequence of Star-Forming Galaxies Across Cosmic Time 

　　   

Speaker: Xianzhong Zheng(PMO)

Time: Thursday, 3:00pm, June 18th

Location: Lecture Hall, 3rd floor  

　　   

Star formation takes place mostly in star-forming galaxies (SFGs) from high-z to the present day. The tight correlation between star formation rates (SFRs) and stellar mass among SFGs, namely the so-called main sequence of SFGs, has become one of the fundamental relationships to verify models of galaxy formation and evolution. Characterizing the slope, normalization and scatter of the main sequence provides key insights into the physical processes regulating star formation in galaxies.  I will present recent observational advances in measuring features of the main sequence of SFGs across cosmic time, and discuss implications for understanding bursty star formation histories of low- and high-mass SFGs,  relative roles of in situ star formation versus mergers in driving galaxy mass assembly, and effects of bulge growth on galaxy star formation  

　　  

SHAO-USTC Lecture  

Title: Probes of Strong gravity

Speaker: Yefei Yuan (USTC)

Time: Friday, 1:30pm,June 19th

Location: Room 1617  

Abstract:   Emission from gas and stars (pulsars) near the event horizon of black hole  could be used as probes of strong gravity of black hole. Especially, emission   from the relativistic accretion disks around black holes could be used to diagnose  both the physical properties of the accretion flow and that of black hole.   Disk emission includes the continuous radiation from disk and its corona, the broad line   emission from an X-ray irradiated disk, and the polarized component from these emissions.   In this lecture, I would like to a brief review on the dynamics of different accretion   flows and how the spectral energy distribution, the line profile and its variability, polarized   emission and even the images of the accretion flow could be used to study the physical   process in strong gravity near the  event horizon of black holes.  

　　    

Group meetings and additional talks  

SHAO SDSS-IV meeting

Time: Wednesday, 3:00 pm, June 17  

 

Location: Room 1714

Title: Chemical Cartography with APOGEE: Metallicity Distribution Functions and the Chemical Structure of the Milky Way Disk

Refs: Hayden et al. (arXiv:1503.02110)

Time: Tuesday, 3:00pm,June 16

Speaker: Zhao-Yu Li  

 

Radio Astrophysics Group Seminar

Location: 1617; Contact: Guangrui Yao < gryao@shao.ac.cn>  

Title: A real-time fast radio burst: polarization detection and multiwavelength follow-up  

Speaker: Rushuang Zhao  

Time: Tuesday, 11:30am, June 16  

 

Stellar Cluster and Galaxy Seminar group seminar  

Location: 1617; Contact: Jian Fu<fujian@shao.ac.cn>  

http://cluster.shao.ac.cn/wiki/index.php/Seminar_Plan 

Title: Hypervelocity Stars, Hills Ejecta, and Other Runaways  

Speaker: John Vicker  

Time: Wednesday, 10:30am, June 17  

 

Cosmology and Galaxy Formation Seminar  

Location: 1714; Contact: Ting Xiao< xiaoting@shao.ac.cn>  

http://202.127.24.6/seminars/index.html  

Title:Characterizing Multi-wavelength Properties for Galaxies via Spatially Resolved Approaches  

Speaker: Yewei Mao (PMO)  

Time: Wednesday, 3:00 pm, June 17