Dr Kyle Oman kyle.a.oman@durham.ac.uk
Associate Professor - Royal Society Dorothy Hodgkin Fellow
A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters
Oman, Kyle A; Bahé, Yannick M; Healy, Julia; Hess, Kelley M; Hudson, Michael J; Verheijen, Marc AW
Authors
Yannick M Bahé
Julia Healy
Kelley M Hess
Michael J Hudson
Marc AW Verheijen
Abstract
We combine orbital information from N-body simulations with an analytic model for star formation quenching and SDSS observations to infer the differential effect of the group/cluster environment on star formation in satellite galaxies. We also consider a model for gas stripping, using the same input supplemented with H I fluxes from the ALFALFA survey. The models are motivated by and tested on the Hydrangea cosmological hydrodynamical simulation suite. We recover the characteristic times when satellite galaxies are stripped and quenched. Stripping in massive (Mvir ∼ 1014.5 M⊙) clusters typically occurs at or just before the first pericentric passage. Lower mass (∼1013.5 M⊙) groups strip their satellites on a significantly longer (by ∼3 Gyr) timescale. Quenching occurs later: Balmer emission lines typically fade ∼3.5 Gyr (5.5 Gyr) after first pericentre in clusters (groups), followed a few hundred Myr later by reddenning in (g − r) colour. These ‘delay timescales’ are remarkably constant across the entire satellite stellar mass range probed (∼109.5–1011 M⊙), a feature closely tied to our treatment of ‘group pre-processing’. The lowest mass groups in our sample (∼1012.5 M⊙) strip and quench their satellites extremely inefficiently: typical timescales may approach the age of the Universe. Our measurements are qualitatively consistent with the ‘delayed-then-rapid’ quenching scenario advocated for by several other studies, but we find significantly longer delay times. Our combination of a homogeneous analysis and input catalogues yields new insight into the sequence of events leading to quenching across wide intervals in host and satellite mass.
Citation
Oman, K. A., Bahé, Y. M., Healy, J., Hess, K. M., Hudson, M. J., & Verheijen, M. A. (2021). A homogeneous measurement of the delay between the onsets of gas stripping and star formation quenching in satellite galaxies of groups and clusters. Monthly Notices of the Royal Astronomical Society, 501(4), 5073-5095. https://doi.org/10.1093/mnras/staa3845
Journal Article Type | Article |
---|---|
Acceptance Date | Dec 12, 2020 |
Online Publication Date | Dec 14, 2021 |
Publication Date | 2021-03 |
Deposit Date | Jan 6, 2021 |
Publicly Available Date | Jan 6, 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 | 501 |
Issue | 4 |
Pages | 5073-5095 |
DOI | https://doi.org/10.1093/mnras/staa3845 |
Public URL | https://durham-repository.worktribe.com/output/1247963 |
Related Public URLs | https://arxiv.org/abs/2009.00667v3 |
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Copyright Statement
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Accepted Journal Article
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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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