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dc.contributor.authorSchawinski, K.
dc.contributor.authorKhochfar, S.
dc.contributor.authorKaviraj, S.
dc.contributor.authorYi, S.K.
dc.contributor.authorLee, Y.-W.
dc.contributor.authorBoselli, A.
dc.contributor.authorDonas, J.
dc.contributor.authorMilliard, B.
dc.contributor.authorBarlow, T.
dc.contributor.authorConrow, T.
dc.contributor.authorForster, K.
dc.contributor.authorFriedman, P.G.
dc.contributor.authorMartin, D.C.
dc.contributor.authorMorrissey, P.
dc.contributor.authorSeibert, M.
dc.contributor.authorSmall, T.
dc.contributor.authorWyder, T.K.
dc.contributor.authorNeff, S.
dc.contributor.authorSchiminovich, D.
dc.contributor.authorBianchi, L.
dc.contributor.authorHeckman, T.
dc.contributor.authorSzalay, A.
dc.contributor.authorMadore, B.
dc.contributor.authorRich, R.M.
dc.date.accessioned2013-10-31T14:01:07Z
dc.date.available2013-10-31T14:01:07Z
dc.date.issued2006-08-24
dc.identifier.citationSchawinski , K , Khochfar , S , Kaviraj , S , Yi , S K , Lee , Y-W , Boselli , A , Donas , J , Milliard , B , Barlow , T , Conrow , T , Forster , K , Friedman , P G , Martin , D C , Morrissey , P , Seibert , M , Small , T , Wyder , T K , Neff , S , Schiminovich , D , Bianchi , L , Heckman , T , Szalay , A , Madore , B & Rich , R M 2006 , ' Suppression of star formation in early-type galaxies by feedback from supermassive black holes ' , Nature , vol. 442 , no. 7105 , pp. 888-891 . https://doi.org/10.1038/nature04934
dc.identifier.issn0028-0836
dc.identifier.otherPURE: 2067825
dc.identifier.otherPURE UUID: 01d55d19-2fe3-4cd5-bcf7-cb6a7f6d4814
dc.identifier.otherScopus: 33747868665
dc.identifier.otherORCID: /0000-0002-5601-575X/work/77850183
dc.identifier.urihttp://hdl.handle.net/2299/11951
dc.description.abstractDetailed high-resolution observations of the innermost regions of nearby galaxies have revealed the presence of supermassive black holes. These black holes may interact with their host galaxies by means of 'feedback' in the form of energy and material jets; this feedback affects the evolution of the host and gives rise to observed relations between the black hole and the host. Here we report observations of the ultraviolet emissions of massive early-type galaxies. We derive an empirical relation for a critical black-hole mass (as a function of velocity dispersion) above which the outflows from these black holes suppress star formation in their hosts by heating and expelling all available cold gas. Supermassive black holes are negligible in mass compared to their hosts but nevertheless seem to play a critical role in the star formation history of galaxies.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofNature
dc.titleSuppression of star formation in early-type galaxies by feedback from supermassive black holesen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre of Data Innovation Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=33747868665&partnerID=8YFLogxK
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1038/nature04934
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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