SHAO Astrophysics Colloquium

Title:   New Observational Perspectives on the Galaxy's Central Bulge/Bar System

Speaker: Mike Rich (UCLA)

Time： 3pm, September 18 (Monday)
Location: Lecture Hall, 3rd floor

Abstract:

The center of the Milky Way hosts 2x10^10 Solar masses of stars in its central 5,000 light years.  This central region is of great interest because the stars have signs of a formation history that is very different from the vicinity of our Sun- a history in which successive generations of supernovae built up the elements we observe today.  I will review what we know about this region and report on new results, from a new map of the velocities of stars that suggests that the

bulge/bar formed from a the buckling of a massive disk, to investigations of the properties of red giant stars lying only 1 parsec from the central black hole, to the global kinematics of red giants hosting SiO maser sources. The unusual characteristics and formation history of this region informs us about the history of galaxy formation in general.

Title:  Toy model for the growth of black holes and galaxy quenching

Speaker: Sandra Faber (UCSC)

Time： 3pm, September 21(Thursday)

Location: Lecture Hall, 3rd floor

Group meetings

Black hole Accretion and High-energy Astrophysics /Black Hole Feedback and Cosmic Ray Astrophysics Seminar

Location: 1608

Time: 14:00-16:00, Wednesday(Sep. 20th)

Speaker: Zhaoming Gan

Title: Simulating the interaction of jets with the intracluster medium

http://adsabs.harvard.edu/abs/2017MNRAS.470.4530W

Speaker: Weixiao Wang
Title: Line-driven disc wind model for ultrafast outflows in active galactic nuclei - scaling with luminosity

http://adsabs.harvard.edu/abs/2017MNRAS.465.2873N