Journal Article

AGN-enhanced outflows of low-ionization gas in star-forming galaxies at 1.7 < <i>z</i> < 4.6

M. Talia, M. Brusa, A. Cimatti, B. C. Lemaux, R. Amorin, S. Bardelli, L. P. Cassarà, O. Cucciati, B. Garilli, A. Grazian, L. Guaita, N. P. Hathi, A. Koekemoer, O. Le Fèvre, D. Maccagni, K. Nakajima, L. Pentericci, J. Pforr, D. Schaerer, E. Vanzella, D. Vergani, G. Zamorani and E. Zucca

in Monthly Notices of the Royal Astronomical Society

Published on behalf of Royal Astronomical Society

Volume 471, issue 4, pages 4527-4540
ISSN: 0035-8711
Published online July 2017 | e-ISSN: 1365-2966 | DOI:
AGN-enhanced outflows of low-ionization gas in star-forming galaxies at 1.7 < z < 4.6

Show Summary Details



Fast and energetic winds are invoked by galaxy formation models as essential processes in the evolution of galaxies. These outflows can be powered either by star formation (SF) and/or active galactic nucleus (AGN) activity, but the relative dominance of the two mechanisms is still under debate. We use spectroscopic stacking analysis to study the properties of the low-ionization phase of the outflow in a sample of 1330 star-forming galaxies (SFGs) and 79 X-ray-detected (1042 < LX < 1045 erg s−1) Type 2 AGN at 1.7 < z < 4.6 selected from a compilation of deep optical spectroscopic surveys, mostly zCOSMOS-Deep and VIMOS Ultra Deep Survey (VUDS). We measure mean velocity offsets of ∼− 150 km s−1 in the SFGs, while in the AGN sample the velocity is much higher (∼− 950 km s−1), suggesting that the AGN is boosting the outflow up to velocities that could not be reached only with the SF contribution. The sample of X-ray AGN has on average a lower SF rate than non-AGN SFGs of similar mass: this, combined with the enhanced outflow velocity in AGN hosts, is consistent with AGN feedback in action. We further divide our sample of AGN into two X-ray luminosity bins: we measure the same velocity offsets in both stacked spectra, at odds with results reported for the highly ionized phase in local AGN, suggesting that the two phases of the outflow may be mixed only up to relatively low velocities, while the highest velocities can be reached only by the highly ionized phase.

Keywords: ISM: jets and outflows; galaxies: active; galaxies: evolution; galaxies: high-redshift – galaxies: ISM; ultraviolet: ISM

Journal Article.  10332 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.