Professor OMAR ALMAINI omar.almaini@nottingham.ac.uk
PROFESSOR OF ASTROPHYSICS
Massive post-starburst galaxies at z > 1 are compact proto-spheroids
Almaini, Omar; Wild, Vivienne; Maltby, David T.; Hartley, William G.; Simpson, Chris; Hatch, Nina A.; McLure, Ross J.; Dunlop, James S.; Rowlands, Kate
Authors
Vivienne Wild
Dr DAVID MALTBY David.Maltby@nottingham.ac.uk
Teaching Associate in Physics andAstronomy
William G. Hartley
Chris Simpson
Professor NINA HATCH nina.hatch@nottingham.ac.uk
PROFESSOR OF ASTRONOMY
Ross J. McLure
James S. Dunlop
Kate Rowlands
Abstract
We investigate the relationship between the quenching of star formation and the structural transformation of massive galaxies, using a large sample of photometrically-selected poststarburst galaxies in the UKIDSS UDS field. We find that post-starburst galaxies at highredshift (z > 1) show high Sérsic indices, significantly higher than those of active star-forming galaxies, but with a distribution that is indistinguishable from the old quiescent population. We conclude that the morphological transformation occurs before (or during) the quenching of star formation. Recently quenched galaxies are also the most compact; we find evidence that massive post-starburst galaxies (M_ > 1010:5 M_) at high redshift (z > 1) are on average smaller than comparable quiescent galaxies at the same epoch. Our findings are consistent with a scenario in which massive passive galaxies are formed from three distinct phases: (1) gas-rich dissipative collapse to very high densities, forming the proto-spheroid; (2) rapid quenching of star formation, to create the “red nugget” with post-starburst features; (3) a gradual growth in size as the population ages, perhaps as a result of minor mergers.
Citation
Almaini, O., Wild, V., Maltby, D. T., Hartley, W. G., Simpson, C., Hatch, N. A., McLure, R. J., Dunlop, J. S., & Rowlands, K. (2017). Massive post-starburst galaxies at z > 1 are compact proto-spheroids. Monthly Notices of the Royal Astronomical Society, 472(2), 1401-1412. https://doi.org/10.1093/mnras/stx1957
Journal Article Type | Article |
---|---|
Acceptance Date | Jul 28, 2017 |
Online Publication Date | Aug 4, 2017 |
Publication Date | 2017-12 |
Deposit Date | Sep 7, 2017 |
Publicly Available Date | Sep 7, 2017 |
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 | 472 |
Issue | 2 |
Pages | 1401-1412 |
DOI | https://doi.org/10.1093/mnras/stx1957 |
Keywords | galaxies: evolution – galaxies: formation – galaxies: fundamental parameters – galaxies: structure – galaxies: high-redshift |
Public URL | https://nottingham-repository.worktribe.com/output/876124 |
Publisher URL | https://academic.oup.com/mnras/article/472/2/1401/4064374/Massive-poststarburst-galaxies-at-zgt1-are-compact |
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. |
Contract Date | Sep 7, 2017 |
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Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf
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