Professor Michele Fumagalli michele.fumagalli@durham.ac.uk
Academic Visitor
MUSE searches for galaxies near very metal-poor gas clouds at z~3: new constraints for cold accretion models
Fumagalli, M.; Cantalupo, S.; Dekel, A.; Morris, S.L.; O'Meara, J.M.; Prochaska, J.X.; Theuns, T.
Authors
S. Cantalupo
A. Dekel
Professor Simon Morris simon.morris@durham.ac.uk
Emeritus Professor
J.M. O'Meara
J.X. Prochaska
T. Theuns
Abstract
We report on the search for galaxies in the proximity of two very metal-poor gas clouds at z ∼ 3 towards the quasar Q0956+122. With a 5-hour Multi-Unit Spectroscopic Explorer (MUSE) integration in a ∼500 × 500 kpc2 region centred at the quasar position, we achieve a ≥80 per cent complete spectroscopic survey of continuum-detected galaxies with mR ≤ 25 mag and Lyα emitters with luminosity LLyα ≥ 3 × 1041 erg s− 1. We do not identify galaxies at the redshift of a z ∼ 3.2 Lyman limit system (LLS) with log Z/Z⊙ = −3.35 ± 0.05, placing this gas cloud in the intergalactic medium or circumgalactic medium of a galaxy below our sensitivity limits. Conversely, we detect five Lyα emitters at the redshift of a pristine z ∼ 3.1 LLS with log Z/Z⊙ ≤ −3.8, while ∼0.4 sources were expected given the z ∼ 3 Lyα luminosity function. Both this high detection rate and the fact that at least three emitters appear aligned in projection with the LLS suggest that this pristine cloud is tracing a gas filament that is feeding one or multiple galaxies. Our observations uncover two different environments for metal-poor LLSs, implying a complex link between these absorbers and galaxy haloes, which ongoing MUSE surveys will soon explore in detail. Moreover, in agreement with recent MUSE observations, we detected a ∼ 90 kpc Lyα nebula at the quasar redshift and three Lyα emitters reminiscent of a ‘dark galaxy’ population.
Citation
Fumagalli, M., Cantalupo, S., Dekel, A., Morris, S., O'Meara, J., Prochaska, J., & Theuns, T. (2016). MUSE searches for galaxies near very metal-poor gas clouds at z~3: new constraints for cold accretion models. Monthly Notices of the Royal Astronomical Society, 462(2), 1978-1988. https://doi.org/10.1093/mnras/stw1782
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 18, 2016 |
Online Publication Date | Jul 25, 2016 |
Publication Date | Oct 21, 2016 |
Deposit Date | Aug 31, 2016 |
Publicly Available Date | Aug 31, 2016 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 462 |
Issue | 2 |
Pages | 1978-1988 |
DOI | https://doi.org/10.1093/mnras/stw1782 |
Public URL | https://durham-repository.worktribe.com/output/1398278 |
Files
Published Journal Article
(1.7 Mb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society ©: 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
Modelling gas around galaxy pairs and groups using the Q0107 quasar triplet
(2023)
Journal Article
Probing the parameters of the intergalactic medium using quasars
(2022)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search