Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. The dense molecular gas in the z ∼ 6 QSO SDSS J231038.88+185519.7 resolved by ALMA
 

The dense molecular gas in the z ∼ 6 QSO SDSS J231038.88+185519.7 resolved by ALMA

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2018
Author(s)
Feruglio, Chiara  
•
Fiore, F.  
•
Carniani, S.
•
Maiolino, R.
•
D'ODORICO, Valentina  
•
Luminari, A.  
•
Barai, P.  
•
Bischetti, M.  
•
BONGIORNO, ANGELA  
•
CRISTIANI, Stefano  
•
Ferrara, A.
•
Gallerani, S.
•
Marconi, Alessandro  
•
Pallottini, A.
•
Piconcelli, E.  
•
ZAPPACOSTA, Luca  
DOI
10.1051/0004-6361/201833174
Abstract
We present ALMA observations of the CO(6-5) and [CII] emission lines and the sub-millimeter continuum of the z ∼ 6 quasi-stellar object (QSO) SDSS J231038.88+185519.7. Compared to previous studies, we have analyzed a synthetic beam that is ten times smaller in angular size, we have achieved ten times better sensitivity in the CO(6-5) line, and two and half times better sensitivity in the [CII] line, enabling us to resolve the molecular gas emission. We obtain a size of the dense molecular gas of 2.9 ± 0.5 kpc, and of 1.4 ± 0.2 kpc for the 91.5 GHz dust continuum. By assuming that CO(6-5) is thermalized, and by adopting a CO to H2 conversion factor αCO = 0.8 M☉K-1 (km s)-1 pc2, we infer a molecular gas mass of M(H2) = (3.2±0.2)×1010 M☉. Assuming that the observed CO velocity gradient is due to an inclined rotating disk, we derive a dynamical mass of Mdynsin2(i)=(2.4 ± 0.5)×1010 M☉, which is a factor of approximately two smaller than the previously reported estimate based on [CII]. Regarding the central black hole, we provide a new estimate of the black hole mass based on the C IV emission line detected in the VLT/X-shooter spectrum: MBH = (1.8 ± 0.5)×109 M☉. We find a molecular gas fraction of μ = M(H2)/M* ∼ 4.4, where M∗ ≈ Mdyn - M(H2) - M(BH). We derive a ratio νrot/σ ≈ 1 - 2 suggesting high gas turbulence, outflows/inflows and/or complex kinematics due to a merger event. We estimate a global Toomre parameter Q ∼ 0.2 - 0.5, indicating likely cloud fragmentation. We compare, at the same angular resolution, the CO(6-5) and [CII] distributions, finding that dense molecular gas is more centrally concentrated with respect to [CII]. We find that the current BH growth rate is similar to that of its host galaxy.

The reduced data cubes and images are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/619/A39

Volume
619
Start page
A39
Uri
http://hdl.handle.net/20.500.12386/27890
Url
https://www.aanda.org/articles/aa/abs/2018/11/aa33174-18/aa33174-18.html
Issn Identifier
0004-6361
Ads BibCode
2018A&A...619A..39F
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

aa33174-18.pdf

Description
Pdf editoriale
Size

1.29 MB

Format

Adobe PDF

Checksum (MD5)

e4da47c456c494f0a77c715720663813

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback