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