The impact of ionized outflows from z - 2.5 quasars is not through instantaneous in situ quenching: The evidence from ALMA and VLT/SINFONI
Artikel i vetenskaplig tidskrift, 2021

We present high-resolution (-2.4 kpc) ALMA band 7 observations (rest-frame λ - 250 μm) of three powerful z - 2.5 quasars (Lbol = 1047.3–1047.5 erg s−1). These targets have previously been reported as showing evidence for suppressed star formation based on cavities in the narrow H α emission at the location of outflows traced with [O III] emission. Here, we combine the ALMA observations with a re-analysis of the VLT/SINFONI data to map the rest-frame far-infrared emission, H α emission, and [O III] emission. In all targets, we observe high velocity [O III] gas (i.e. W80 - 1000–2000 km s−1) across the whole galaxy. We do not identify any H α emission that is free from contamination from AGN-related processes; however, based on SED analyses, we show that the ALMA data contain a significant dust-obscured star formation component in two out of the three systems. This dust emission is found to be extended over ≈1.5–5.5 kpc in the nuclear regions, overlaps with the previously reported H α cavities and is co-spatial with the peak in surface brightness of the [O III] outflows. In summary, within the resolution and sensitivity limits of the data, we do not see any evidence for a instantaneous shut down of in situ star formation caused directly by the outflows. However, similar to the conclusions of previous studies and based on our measured star formation rates, we do not rule out that the global host galaxy star formation could be suppressed on longer time-scales by the cumulative effect of quasar episodes during the growth of these massive black holes.

X-rays: galaxies

Galaxies: evolution

Infrared: galaxies

Galaxies: active

Författare

Jan Scholtz

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Durham University

C. M. Harrison

Newcastle University

D. J. Rosario

Durham University

D. M. Alexander

Durham University

Kirsten Kraiberg Knudsen

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

Flora Stanley

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

C. C. Chen

Academia Sinica

D. Kakkad

European Southern Observatory Santiago

V. Mainieri

European Southern Observatory (ESO)

J. R. Mullaney

University of Sheffield

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 505 4 5469-5487

Ämneskategorier

Astronomi, astrofysik och kosmologi

DOI

10.1093/mnras/stab1631

Mer information

Senast uppdaterat

2021-07-22