Skip to main content

Research Repository

Advanced Search

MUSE Analysis of Gas around Galaxies (MAGG) - II: Metal-enriched halo gas around z ∼ 1 galaxies

Dutta, Rajeshwari; Fumagalli, Michele; Fossati, Matteo; Lofthouse, Emma K.; Prochaska, J. Xavier; Battaia, Fabrizio Arrigoni; Bielby, Richard M.; Cantalupo, Sebastiano; Cooke, Ryan J.; Murphy, Michael T.; O’Meara, John M.

MUSE Analysis of Gas around Galaxies (MAGG) - II: Metal-enriched halo gas around z ∼ 1 galaxies Thumbnail


Authors

Rajeshwari Dutta

Matteo Fossati

Emma K. Lofthouse

J. Xavier Prochaska

Fabrizio Arrigoni Battaia

Richard M. Bielby

Sebastiano Cantalupo

Michael T. Murphy

John M. O’Meara



Abstract

We present a study of the metal-enriched cool halo gas traced by Mg II absorption around 228 galaxies at z ∼ 0.8–1.5 within 28 quasar fields from the MUSE Analysis of Gas around Galaxies survey. We observe no significant evolution in the Mg II equivalent width versus impact parameter relation and in the Mg II covering fraction compared to surveys at z ≲ 0.5. The stellar mass, along with distance from galaxy centre, appears to be the dominant factor influencing the Mg II absorption around galaxies. With a sample that is 90 per cent complete down to a star formation rate of ≈0.1 M⊙yr−1 and up to impact parameters ≈250–350 kpc from quasars, we find that the majority (⁠67+12−15 per cent or 14/21) of the Mg II absorption systems are associated with more than one galaxy. The complex distribution of metals in these richer environments adds substantial scatter to previously reported correlations. Multiple galaxy associations show on average five times stronger absorption and three times higher covering fraction within twice the virial radius than isolated galaxies. The dependence of Mg II absorption on galaxy properties disfavours the scenario in which a widespread intragroup medium dominates the observed absorption. This leaves instead gravitational interactions among group members or hydrodynamic interactions of the galaxy haloes with the intragroup medium as favoured mechanisms to explain the observed enhancement in the Mg II absorption strength and cross-section in rich environments.

Citation

Dutta, R., Fumagalli, M., Fossati, M., Lofthouse, E. K., Prochaska, J. X., Battaia, F. A., Bielby, R. M., Cantalupo, S., Cooke, R. J., Murphy, M. T., & O’Meara, J. M. (2020). MUSE Analysis of Gas around Galaxies (MAGG) - II: Metal-enriched halo gas around z ∼ 1 galaxies. Monthly Notices of the Royal Astronomical Society, 499(4), 5022-5046. https://doi.org/10.1093/mnras/staa3147

Journal Article Type Article
Acceptance Date Oct 9, 2020
Online Publication Date Oct 12, 2020
Publication Date 2020-12
Deposit Date Oct 13, 2020
Publicly Available Date Nov 17, 2020
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 499
Issue 4
Pages 5022-5046
DOI https://doi.org/10.1093/mnras/staa3147
Public URL https://durham-repository.worktribe.com/output/1259652

Files

Published Journal Article (4.3 Mb)
PDF

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.






You might also like



Downloadable Citations