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dc.contributor.authorThomas, D.
dc.contributor.authorMaraston, C.
dc.contributor.authorSchawinski, K.
dc.contributor.authorJoo, S.-J.
dc.contributor.authorKaviraj, S.
dc.contributor.authorSarzi, M.
dc.contributor.authorYi, S.K.
dc.date.accessioned2013-12-17T13:00:09Z
dc.date.available2013-12-17T13:00:09Z
dc.date.issued2006-12-01
dc.identifier.citationThomas , D , Maraston , C , Schawinski , K , Joo , S-J , Kaviraj , S , Sarzi , M & Yi , S K 2006 , ' Environment and the epochs of galaxy formation in the SDSS era ' , Proceedings of the International Astronomical Union , vol. 2 , no. S241 , pp. 546-550 . https://doi.org/10.1017/S1743921307009088
dc.identifier.issn1743-9213
dc.identifier.otherPURE: 2067953
dc.identifier.otherPURE UUID: ef40c897-b5b8-4183-8ae0-f976b505da61
dc.identifier.otherScopus: 37149030657
dc.identifier.urihttp://hdl.handle.net/2299/12373
dc.description.abstractWe analyse a sample of 1,652 elliptical galaxies morphologically selected from the SDSS DR4 with respect to their stellar population properties such as luminosity weighted ages, metallicities and /Fe element abundance ratios. We confirm and statistically strengthen earlier results that all three stellar population parameters correlate with velocity dispersion, hence galaxy mass. Most surprisingly and differently from previous work, however, these scaling relations turn out to be independent of environmental density for the bulk of the population. This implies that the formation epochs and timescales of the stellar populations in massive galaxies are entirely independent of the environmental density and only driven by galaxy mass. At the low-mass end some fraction of the galaxies show signs of recent star formation on top of the general downsizing trend. It is only the fractional amount of such rejuvenated galaxies that reveals strong dependence with environment. The influence of the environment apparently undergoes a phase transition at about z 1. An early galaxy formation phase without environmental dependence is followed by a rejuvenation phase at redshifts below z 1 affecting mostly low-mass galaxies, during which the environment plays a crucial role.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofProceedings of the International Astronomical Union
dc.titleEnvironment and the epochs of galaxy formation in the SDSS eraen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=37149030657&partnerID=8YFLogxK
rioxxterms.versionofrecordhttps://doi.org/10.1017/S1743921307009088
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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