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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
- 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
- Subjects :
- quasars emission lines
Astrophysics::High Energy Astrophysical Phenomena
galaxies active
FOS: Physical sciences
Context (language use)
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
intergalactic medium
quasars individual SDSS153830
55+085517
0
0103 physical sciences
Astrophysics::Solar and Stellar Astrophysics
Emission spectrum
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
Intergalactic medium
Physics
Nebula
active
quasars: emission lines
quasars: individual: SDSS 153830.55+085517.0 [galaxies]
010308 nuclear & particles physics
Quasars: individual: SDSS 153830.55+085517.0
Quasars: emission line
Velocity dispersion
Astronomy and Astrophysics
Quasar
Galaxies: active
Astrophysics - Astrophysics of Galaxies
Redshift
Galaxy
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
Intergalactic travel
quasars emission line
Subjects
Details
- Language :
- English
- Database :
- OpenAIRE
- Journal :
- Astronomy & Astrophysics, 635
- Accession number :
- edsair.doi.dedup.....b6fd8bc89b2ca0e8234d81721216b35a