Speaker
Maximilian Eisenreich
(MPA)
Description
We use hydrodynamical simulations to study the influence of AGN accretion and feedback on the late morphological and kinematic evolution of the hot and cold interstellar medium and young stars in isolated early-type galaxies (ETGs). The complex interplay of gas cooling from a hot halo, feedback from star formation (metal and energy return from supernova Ia and II, AGB winds) and gas accretion onto and feedback (kinetic and radiative) from the central AGN is investigated. We present the most prominent signatures of AGN feedback on the kinematics and phase distribution of the gas, it's metal distribution, and the stellar population.
Author
Maximilian Eisenreich
(MPA)