Evidence for powerful AGN winds at high redshift: Dynamics of galactic outflows in radio galaxies during the "Quasar Era"
arXiv:0809.5171 · doi:10.1051/0004-6361:200810346
Abstract
AGN feedback now appears as an attractive mechanism to resolve some of the outstanding problems with the "standard" cosmological models, in particular those related to massive galaxies. To directly constrain how this may influence the formation of massive galaxies near the peak in the redshift distribution of powerful quasars, z~2, we present an analysis of the emission-line kinematics of 3 powerful radio galaxies at z~2-3 (HzRGs) based on rest-frame optical integral-field spectroscopy obtained with SINFONI on the VLT. HzRGs are among the most massive galaxies, so AGN feedback may have a particularly clear signature. We find evidence for bipolar outflows in all HzRGs, with kinetic energies that are equivalent to 0.2% of the rest-mass of the supermassive black hole. Velocity offsets in the outflows are ~800-1000 km s^-1 between the blueshifted and redshifted line emission, FWHMs ~1000 km s^-1 suggest strong turbulence. Ionized gas masses estimated from the Ha luminosity are of order 10^10 M_s, similar to the molecular gas content of HzRGs, underlining that these outflows may indicate a significant phase in the evolution of the host galaxy. The total energy release of ~10^60 erg during a dynamical time of ~10^7 yrs corresponds to about the binding energy of a massive galaxy. Geometry, timescales and energy injection rates of order 10% of the kinetic energy flux of the jet suggest that the outflows are most likely driven by the radio source. The global energy density release of ~10^57 erg s^-1 Mpc^-3 may also influence the subsequent evolution of the HzRG by enhancing the entropy and pressure in the surrounding halo and facilitating ram-pressure stripping of gas in satellite galaxies that may contribute to the subsequent mass assembly of the HzRG through low-dissipation "dry" mergers.
A&A in press, minor edits & typo in table captions 2-4
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- The XMM-Newton and NuSTAR view of IRASF11119+3257. I Detection of multiple UFO components and a very cold corona
- The extended narrow-line region of two type-I quasi-stellar objects
- The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT continuum observations
- A large thermal energy reservoir in the nascent intracluster medium at a redshift of 4.3
- The Complex X-ray Obscuration Environment in the Radio Loud Type 2 Quasar 3C 223
- The host galaxies of radio-loud AGN: colour structure
- Feedback Factory: Multiple faint radio-jets detected in a cluster at z=2
- ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193
- Broad [CII] line wings as tracer of molecular and multi-phase outflows in infrared bright galaxies
- ATCA detections of massive molecular gas reservoirs in dusty, high-z radio galaxies
- Detection of helicoidal motion in the optical jet of PKS 0521-365
- Hunting for the nature of the enigmatic narrow-line Seyfert 1 galaxy PKS 2004-447
- Acoustic waves and g-mode turbulence as energy carriers in a viscous intracluster medium
- Modelling observable signatures of jet-ISM interaction: thermal emission and gas kinematics
- Exploring the gaseous halos of z>3 radio galaxies with UVES and JWST/NIRSpec