Abstract
Recent observations have revealed nuclear outflows in high-redshift, star
forming galaxies. We study outflows driven by Active Galactic Nuclei (AGNs)
using high- resolution simulations of idealized z=2 isolated disk galaxies.
Episodic accretion events lead to outflows with velocities >1000 km/s and mass
outflow rates up to the star formation rate (several tens of Msun/yr).
Outflowing winds escape perpendicular to the disk with wide opening angles, and
are typically asymmetric (i.e. unipolar) because dense gas above or below the
AGN in the resolved disk inhibits outflow. Owing to rapid variability in the
accretion rates, outflowing gas may be detectable even when the AGN is
effectively öff." The highest velocity outflows are concentrated within 2-3
kpc of the galactic center during the peak accretion. With our purely thermal
AGN feedback model -- standard in previous literature -- the outflowing
material is mostly hot (10^6 K) and diffuse (nH<10^(-2) cm-3), but includes a
cold component entrained in the hot wind. Despite the powerful bursts and
outflow rates near the star formation rate, AGN feedback has little effect on
the dense gas in the galaxy disk.
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