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The WISSH quasars project: VIII. Outflows and metals in the circum-galactic medium around the hyper-luminous z ∼ 3.6 quasar J1538+08

Authors :
M. Bischetti
Sebastiano Cantalupo
F. Duras
Michele Ginolfi
Enrico Piconcelli
Fabrizio Fiore
Chiara Feruglio
A. Travascio
C. Vignali
G. Vietri
F. Arrigoni Battaia
Luca Zappacosta
Valentina D'Odorico
Angela Bongiorno
Travascio, A
Zappacosta, L
Cantalupo, S
Piconcelli, E
Arrigoni Battaia, F
Ginolfi, M
Bischetti, M
Vietri, G
Bongiorno, A
D'Odorico, V
Duras, F
Feruglio, C
Vignali, C
Fiore, F
Travascio, A.
Zappacosta, Luca
Cantalupo, S.
Piconcelli, Enrico
Arrigoni Battaia, F.
Ginolfi, M.
Bischetti, Manuela
Vietri, Giustina
Bongiorno, Angela
D'Odorico, Valentina
Duras, Federica
Feruglio, Chiara
Vignali, C.
Fiore, Fabrizio
Travascio A.
Zappacosta L.
Cantalupo S.
Piconcelli E.
Arrigoni Battaia F.
Ginolfi M.
Bischetti M.
Vietri G.
Bongiorno A.
D'Odorico V.
Duras F.
Feruglio C.
Vignali C.
Fiore F.
ITA
DEU
CHE
Source :
Astronomy & Astrophysics, 635
Publication Year :
2020
Publisher :
EDP Sciences, 2020.

Abstract

During the last years, Ly$\alpha$ nebulae have been routinely detected around high-z, radio-quiet quasars (RQQs) thanks to the advent of sensitive integral field spectrographs. Constraining the physical properties of the Ly$\alpha$ nebulae is crucial for a full understanding of the circum-galactic medium (CGM), which is a venue of feeding and feedback processes. The most luminous quasars are privileged test-beds to study these processes, given their large ionizing fluxes and dense CGM environments in which they are expected to be embedded. We aim at characterizing the rest-frame UV emission lines in the CGM around a hyper-luminous, broad emission line, RQQ at z~3.6, that exhibits powerful outflows at both nuclear and host galaxy scales. We analyze VLT/MUSE observations of the quasar J1538+08 and perform a search for extended UV emission lines to characterize its morphology, emissivity, kinematics and metal content. We report the discovery of a very luminous ($\sim2 \times10^{44}~erg~s^{-1}$), giant Ly$\alpha$ nebula and a likely associated extended CIV nebula. The Ly$\alpha$ nebula emission exhibits moderate blueshift compared with the quasar systemic redshift and large average velocity dispersion ($\sigma_{v}$ ~700 $km~s^{-1}$) across the nebula, while the CIV nebula shows $\sigma_{v}$~$350~km~s^{-1}$. The Ly$\alpha$ line profile exhibits a significant asymmetry towards negative velocity values at 20-30 kpc south of the quasar and is well parameterized by two Gaussian components: a narrow ($\sigma$~$470~km~s^{-1}$) systemic one plus a broad ($\sigma$~1200 $km~s^{-1}$), blueshifted (~1500 $km~s^{-1}$) one. Our analysis of the MUSE observation of J1538+08 reveals metal-enriched CGM around this hyper-luminous quasar and our detection of blueshifted emission in the line profile of the Ly$\alpha$ nebula suggests that powerful nuclear outflows can propagate through the CGM over tens of kpc.<br />Comment: 14 pages, 16 figures, 2 tables. Accepted for publication in A&A Journal

Details

Language :
English
Database :
OpenAIRE
Journal :
Astronomy & Astrophysics, 635
Accession number :
edsair.doi.dedup.....b6fd8bc89b2ca0e8234d81721216b35a