The Impact of Positive AGN Feedback on the Properties of Galaxies in a Semi-Analytic Model of Galaxy Formation
arxiv(2024)
摘要
We introduce the state-of-the-art semi-analytic model FEGA (Formation and
Evolution of GAlaxies), which incorporates updated prescriptions for key
physical processes in galaxy formation. Notably, FEGA features an unprecedented
semi-analytic modeling of positive Active Galactic Nuclei (AGN) feedback. The
model combines the latest prescriptions for gas infall and cooling, a revised
star formation recipe that incorporates the extended Kennicutt-Schmidt
relation, disk instability, updated supernovae feedback, reincorporation of
ejected gas, hot gas stripping from satellite galaxies, and the formation of
diffuse light. A novel description of AGN feedback is introduced, describing
the positive mode as a burst of star formation from a cooling gas fraction.
FEGA is rigorously calibrated using an MCMC procedure to match the evolution of
the stellar mass and K-band luminosity functions from high redshift to the
present, and the local black hole-bulge mass relation. Subsequently, the model
is tested against several observed and predicted scaling relations, including
the star formation rate-mass, black hole-bulge and stellar mass,
stellar-to-halo mass, and red fraction-mass relations. Additionally, we test
FEGA against other galaxy properties such as the distribution of specific star
formation rates, stellar metallicity and morphology. Our results demonstrate
that the inclusion of positive AGN feedback can co-exist with its negative
counterpart without drastic alterations to other prescriptions. Importantly,
this inclusion improves the ability of the model to describe the primary
scaling relations observed in galaxies.
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