K. Kelkar
Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey
Kelkar, K.; Arag�n-Salamanca, A.; Gray, M.E.; Maltby, D.; Vulcani, B.; De Lucia, G.; Poggianti, B.M.; Zaritsky, D.
Authors
Professor ALFONSO ARAGON-SALAMANCA ALFONSO.ARAGON@NOTTINGHAM.AC.UK
Professor of Astronomy
MEGHAN GRAY MEGHAN.GRAY@NOTTINGHAM.AC.UK
Professor of Astronomy
Dr. DAVID MALTBY David.Maltby@nottingham.ac.uk
Teaching Associate in Physics Andastronomy
B. Vulcani
G. De Lucia
B.M. Poggianti
D. Zaritsky
Abstract
In order to assess whether the environment has a significant effect on galaxy sizes, we compare the mass–size relations of cluster and field galaxies in the 0.4
Citation
Kelkar, K., Aragón-Salamanca, A., Gray, M., Maltby, D., Vulcani, B., De Lucia, G., …Zaritsky, D. (2015). Galaxy sizes as a function of environment at intermediate redshift from the ESO Distant Cluster Survey. Monthly Notices of the Royal Astronomical Society, 450(2), https://doi.org/10.1093/mnras/stv670
Journal Article Type | Article |
---|---|
Acceptance Date | Mar 25, 2015 |
Publication Date | Jun 1, 2015 |
Deposit Date | Apr 20, 2017 |
Publicly Available Date | Apr 20, 2017 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 0035-8711 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 450 |
Issue | 2 |
DOI | https://doi.org/10.1093/mnras/stv670 |
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/750578 |
Publisher URL | https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stv670 |
Additional Information | This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society Published by Oxford University Press on behalf of the Royal Astronomical Society. |
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