Abstract:

 It is well known that Active Galactic Nuclei (AGN) has feedback on galaxies. Previous studies have often focused on gas dynamics and star formation rates in galaxies. However, the kinematics of stars can also be influenced by the feedback processes. In this talk, we will primarily focus on the impact of massive, fast outflows on the dynamics of galactic bulges. We consider both the changes in gravitational potential induced by gas motion and the effects of stellar encounters. Our preliminary findings reveal that the bulge exhibits quasi-periodic radial oscillations, in response to AGN’s activity.

 

个人简介：

彭岳昌，男，2025年毕业于中国科学院高能物理研究所。主要兴趣方向为星系动力学，吸积盘动力学，以及黑洞物理。

Yue-Chang Peng earned his PhD degree from the Institute of High Energy Physics, CAS Beijing in 2025. His main interests are galactic dynamics, accretion disk dynamics, and black hole physics.