Speaker
Fulai Guo
(Shanghai Astronomical Observatory)
Description
AGN and stellar feedback processes strongly affect galaxy formation and are one central unsolved problem in contemporary astronomy. Galactic feedback processes mainly evolve in the circumgalactic medium (CGM), which is another hot research field in recent years. Here I will talk about a series of our recent and ongoing works on both AGN and stellar feedback in the Milky way and several nearby galaxies. By using idealized hydrodynamic simulations and detailed comparisons with multi-wavelength observations, we try to reveal the fundamental physics governing the evolution and impact of these feedback processes.
Primary author
Fulai Guo
(Shanghai Astronomical Observatory)
