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The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet

Beckett, Alexander; Morris, Simon L; Fumagalli, Michele; Bielby, Rich; Tejos, Nicolas; Schaye, Joop; Jannuzi, Buell; Cantalupo, Sebastiano

The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet Thumbnail


Authors

Rich Bielby

Nicolas Tejos

Joop Schaye

Buell Jannuzi

Sebastiano Cantalupo



Abstract

We study the distribution and dynamics of the circumgalactic and intergalactic medium using a dense galaxy survey covering the field around the Q0107 system, a unique z ≈ 1 projected quasar triplet. With full Ly α coverage along all three lines-of-sight from z = 0.18 to z = 0.73, more than 1200 galaxy spectra, and two MUSE fields, we examine the structure of the gas around galaxies on 100–1000 kpc scales. We search for H I absorption systems occurring at the same redshift (within 500 km s−1) in multiple sightlines, finding with >99.9 per cent significance that these systems are more frequent in the observed quasar spectra than in a randomly distributed population of absorbers. This is driven primarily by absorption with column densities N(H I) > 1014 cm−2, whilst multi-sightline absorbers with lower column densities are consistent with a random distribution. Star-forming galaxies are more likely to be associated with multi-sightline absorption than quiescent galaxies. HST imaging provides inclinations and position angles for a subset of these galaxies. We observe a bimodality in the position angle of detected galaxy-absorber pairs, again driven mostly by high-column-density absorbers, with absorption preferentially along the major and minor axes of galaxies out to impact parameters of several hundred kpc. We find some evidence supporting a disc/outflow dichotomy, as H I absorbers near the projected major axis of a galaxy show line-of-sight velocities that tend to align with the rotation of that galaxy, whilst minor-axis absorbers are twice as likely to exhibit O VI at the same redshift.

Citation

Beckett, A., Morris, S. L., Fumagalli, M., Bielby, R., Tejos, N., Schaye, J., …Cantalupo, S. (2021). The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet. Monthly Notices of the Royal Astronomical Society, 506(2), 2574-2602. https://doi.org/10.1093/mnras/stab1630

Journal Article Type Article
Acceptance Date May 26, 2021
Online Publication Date Jun 10, 2021
Publication Date 2021-09
Deposit Date Aug 23, 2021
Publicly Available Date Aug 23, 2021
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 506
Issue 2
Pages 2574-2602
DOI https://doi.org/10.1093/mnras/stab1630
Public URL https://durham-repository.worktribe.com/output/1243357

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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2020 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.






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