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  5. Molecular outflow and feedback in the obscured Quasar XID2028 revealed by ALMA
 

Molecular outflow and feedback in the obscured Quasar XID2028 revealed by ALMA

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2018
Author(s)
Brusa, M.
•
CRESCI, GIOVANNI  
•
E. Daddi
•
Paladino, Rosita  
•
M. Perna
•
BONGIORNO, ANGELA  
•
E. Lusso
•
M. T. Sargent
•
CASASOLA, VIVIANA  
•
Feruglio, Chiara  
•
F. Fraternali
•
I. Georgiev
•
V. Mainieri
•
S. Carniani
•
COMASTRI, Andrea  
•
F. Duras
•
F. Fiore
•
MANNUCCI, FILIPPO  
•
Marconi, Alessandro  
•
PICONCELLI, Enrico  
•
G. Zamorani
•
GILLI, Roberto  
•
F. La Franca
•
LANZUISI, Giorgio  
•
D. Lutz
•
SANTINI, Paola  
•
N. Z. Scoville
•
C. Vignali
•
F. Vito
•
S. Rabien
•
BUSONI, LORENZO  
•
BONAGLIA, MARCO  
DOI
10.1051/0004-6361/201731641
Abstract
We imaged with ALMA and ARGOS/LUCI the molecular gas and the dust and stellar continuum in XID2028, an obscured QSO at z=1.593, where the presence of a massive outflow in the ionized gas component traced by the [O III]5007 emission has been resolved up to 10 kpc. This target represents a unique test case to study QSO 'feedback in action' at the peak epoch of AGN-galaxy coevolution. The QSO has been detected in the CO(5-4) transition and in the 1.3mm continuum, at ~30 and ~20 {\sigma} significance respectively, with both emissions confined in the central (<4 kpc) radius area. Our analysis suggests the presence of a fast rotating molecular disc (v~400 km/s) on very compact scales, and well inside the galaxy extent seen in the rest-frame optical light (~10 kpc, as inferred from the LUCI data). Adding available measurements in additional two CO transitions, CO(2-1) and CO(3-2), we could derive a total gas mass of ~10$^{10}$ M$_\odot$, thanks to a critical assessment of CO excitation and the comparison with Rayleigh-Jeans continuum estimate. This translates into a very low gas fraction (<5%) and depletion time scales of 40-75 Myr, reinforcing the result of atypical gas consumption conditions in XID2028, possibly due to feedback effects on the host galaxy. Finally, we also detect at ~5{\sigma} the presence of high velocity CO gas, which we interpret as a signature of galaxy-scale molecular outflow, spatially coincident with the ionised gas outflow. XID2028 represents therefore a unique case where the measurement of total outflowing mass (~500-800 M$_\odot$/yr) including the molecular and atomic components, in both the ionised and neutral phases, has been attempted for a high-z QSO.
Volume
612
Start page
A29
Uri
http://hdl.handle.net/20.500.12386/29604
Url
https://www.aanda.org/articles/aa/full_html/2018/04/aa31641-17/aa31641-17.html
Issn Identifier
0004-6361
Ads BibCode
2018A&A...612A..29B
Rights
open.access
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R03_Brusa_2018.pdf

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