Kshitija Kelkar
The time delay between star formation quenching and morphological transformation of galaxies in clusters: a phase–space view of EDisCS
Kelkar, Kshitija; Gray, Meghan E; Arag�n-Salamanca, Alfonso; Rudnick, Gregory; Jaff�, Yara L; Jablonka, Pascale; Moustakas, John; Milvang-Jensen, Bo
Authors
MEGHAN GRAY MEGHAN.GRAY@NOTTINGHAM.AC.UK
Professor of Astronomy
Professor ALFONSO ARAGON-SALAMANCA ALFONSO.ARAGON@NOTTINGHAM.AC.UK
Professor of Astronomy
Gregory Rudnick
Yara L Jaff�
Pascale Jablonka
John Moustakas
Bo Milvang-Jensen
Abstract
We explore the possible effect of cluster environments on the structure and star formation histories of galaxies by analysing the projected phase–space (PPS) of intermediate-redshift clusters (0.4 z 0.8). HST I−band imaging data from the ESO Distant Cluster Survey (EDisCS) allow us to measure deviations of the galaxies' light distributions from symmetric and smooth profiles using two parameters, A res ('asymmetry') and RF F (residual flux fraction or 'roughness'). Combining these structural parameters with age-sensitive spectral indicators (H δA , H γA and D n 4000), we establish that in all environments younger star-forming galaxies of all morphologies are 'rougher' and more asymmetric than older, more quiescent ones. Combining a subset of the EDisCS clusters we construct a stacked PPS diagram and find a significant correlation between the position of the galaxies on the PPS and their stellar ages, irrespective of their morphology. We also observe an increasing fraction of galaxies with older stellar populations towards the cluster core, while the galaxies structural parameters (A res and RF F) do not seem to segregate strongly with PPS. These results may imply that, under the possible influence of their immediate cluster environment, galaxies have their star formation suppressed earlier, while their structural transformation happens on a longer timescale as they accumulate and age in the cluster cores.
Citation
Kelkar, K., Gray, M. E., Aragón-Salamanca, A., Rudnick, G., Jaffé, Y. L., Jablonka, P., …Milvang-Jensen, B. (2019). The time delay between star formation quenching and morphological transformation of galaxies in clusters: a phase–space view of EDisCS. Monthly Notices of the Royal Astronomical Society, 486(1), 868-884. https://doi.org/10.1093/mnras/stz905
Journal Article Type | Article |
---|---|
Acceptance Date | Mar 27, 2019 |
Online Publication Date | Mar 28, 2019 |
Publication Date | Jun 1, 2019 |
Deposit Date | Apr 9, 2019 |
Publicly Available Date | Apr 9, 2019 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 486 |
Issue | 1 |
Pages | 868-884 |
DOI | https://doi.org/10.1093/mnras/stz905 |
Keywords | galaxies: clusters: general, galaxies: elliptical and lenticular, cD, galaxies: evolution, galaxies: fundamental parameters, galaxies: spiral, galaxies: statistics |
Public URL | https://nottingham-repository.worktribe.com/output/1770723 |
Publisher URL | https://academic.oup.com/mnras/article/486/1/868/5421638 |
Contract Date | Apr 9, 2019 |
Files
1904.00466 AAS
(1.1 Mb)
PDF
You might also like
Linking the structural properties of galaxies and their star formation histories with STAGES
(2015)
Journal Article
nIFTy galaxy cluster simulations – V. Investigation of the cluster infall region
(2016)
Journal Article
Downloadable Citations
About Repository@Nottingham
Administrator e-mail: discovery-access-systems@nottingham.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 © 2024
Advanced Search