C. d. P. Lagos
Quantifying the impact of mergers on the angular momentum of simulated galaxies
Lagos, C. d. P.; Stevens, A.R.H.; Bower, R.G.; Davis, T.A.; Contreras, S.; Padilla, N.D.; Obreschkow, D.; Croton, D.; Trayford, J.W.; Welker, C.; Theuns, T.
Authors
A.R.H. Stevens
R.G. Bower
T.A. Davis
S. Contreras
N.D. Padilla
D. Obreschkow
D. Croton
J.W. Trayford
C. Welker
Professor Tom Theuns tom.theuns@durham.ac.uk
Professor
Abstract
We use EAGLE to quantify the effect galaxy mergers have on the stellar specific angular momentum of galaxies, jstars. We split mergers into dry (gas-poor)/wet (gas-rich), major/minor and different spin alignments and orbital parameters. Wet (dry) mergers have an average neutral gas-to-stellar mass ratio of 1.1 (0.02), while major (minor) mergers are those with stellar mass ratios ≥0.3 (0.1–0.3). We correlate the positions of galaxies in the jstars–stellar mass plane at z = 0 with their merger history, and find that galaxies of low spins suffered dry mergers, while galaxies of normal/high spins suffered predominantly wet mergers, if any. The radial jstars profiles of galaxies that went through dry mergers are deficient by ≈0.3 dex at r ≲ 10 r50 (with r50 being the half-stellar mass radius), compared to galaxies that went through wet mergers. Studying the merger remnants reveals that dry mergers reduce jstars by ≈30 per cent, while wet mergers increase it by ≈10 per cent, on average. The latter is connected to the build-up of the bulge by newly formed stars of high rotational speed. Moving from minor to major mergers accentuates these effects. When the spin vectors of the galaxies prior to the dry merger are misaligned, jstars decreases by a greater magnitude, while in wet mergers corotation and high orbital angular momentum efficiently spun-up galaxies. We predict what would be the observational signatures in the jstars profiles driven by dry mergers: (i) shallow radial profiles and (ii) profiles that rise beyond ≈10 r50, both of which are significantly different from spiral galaxies.
Citation
Lagos, C. D. P., Stevens, A., Bower, R., Davis, T., Contreras, S., Padilla, N., …Theuns, T. (2018). Quantifying the impact of mergers on the angular momentum of simulated galaxies. Monthly Notices of the Royal Astronomical Society, 473(4), 4956-4974. https://doi.org/10.1093/mnras/stx2667
Journal Article Type | Article |
---|---|
Acceptance Date | Oct 6, 2017 |
Online Publication Date | Oct 14, 2017 |
Publication Date | Feb 1, 2018 |
Deposit Date | Jan 16, 2018 |
Publicly Available Date | Jan 17, 2018 |
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 | 473 |
Issue | 4 |
Pages | 4956-4974 |
DOI | https://doi.org/10.1093/mnras/stx2667 |
Public URL | https://durham-repository.worktribe.com/output/1341390 |
Related Public URLs | https://arxiv.org/abs/1701.04407 |
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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2017 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
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