Show simple item record

dc.contributor.authorKaviraj, S.
dc.contributor.authorCrockett, R.M.
dc.contributor.authorSilk, J.
dc.contributor.authorEllis, R.S.
dc.contributor.authorYi, S.K.
dc.contributor.authorO'Connell, R.W.
dc.contributor.authorWindhorst, R.
dc.contributor.authorWhitmore, B.C.
dc.date.accessioned2014-10-02T11:30:53Z
dc.date.available2014-10-02T11:30:53Z
dc.date.issued2011-09
dc.identifier.citationKaviraj , S , Crockett , R M , Silk , J , Ellis , R S , Yi , S K , O'Connell , R W , Windhorst , R & Whitmore , B C 2011 , Minor-merger-driven growth of early-type galaxies over the last 8 billion years . in Spectral Energy Distribution of Galaxies . Procs IAU Symposium , no. 284 , vol. 7 , Cambridge University Press , pp. 460-464 . https://doi.org/10.1017/S1743921312009623
dc.identifier.isbn9781107019843
dc.identifier.otherPURE: 2066408
dc.identifier.otherPURE UUID: aa2bf767-fb07-4009-a6df-36e7ca40fe18
dc.identifier.otherScopus: 84865677646
dc.identifier.urihttp://hdl.handle.net/2299/14529
dc.description.abstractWe summarise recent progress in understanding the star formation activity in early-type galaxies (ETGs), using recent studies that leverage photometry in the rest-frame ultraviolet (UV) wavelengths. While classically thought to be old, passively-evolving systems, recent UV studies have revealed widespread star formation in ETGs, with ∼20% of the stellar mass in today's ETGs forming at late epochs (z <1). A strong correlation is found between the presence of morphological disturbances and blue UV colours, suggesting that the star formation is merger-driven. However, the major merger rate at late epochs is far too low to satisfy the number of disturbed ETGs, indicating that minor mergers drive the star formation in these galaxies over the latter half of cosmic time. Together with the recent literature which suggests that minor mergers may drive the size evolution of massive ETGs, these results highlight the significant role of minor mergers in driving the evolution of massive galaxies in the low and intermediate-redshift Universe.en
dc.format.extent5
dc.language.isoeng
dc.publisherCambridge University Press
dc.relation.ispartofSpectral Energy Distribution of Galaxies
dc.relation.ispartofseriesProcs IAU Symposium
dc.titleMinor-merger-driven growth of early-type galaxies over the last 8 billion yearsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1017/S1743921312009623
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record