The evolution of QSO spectra

dc.contributor.authorFrancis, Paul
dc.contributor.authorKoratkar, Anuradha
dc.date.accessioned2018-09-10T01:59:35Z
dc.date.available2018-09-10T01:59:35Z
dc.date.issued1995
dc.description.abstractWe study the rest-frame UV spectra of two samples of QSOs, a low-redshift (z~0.4) sample drawn from the IUE archives, and a high-redshift (z~2.2), optically selected sample, the Large Bright QSO Survey (LBQS). The samples overlap substantially in their range of absolute magnitudes and radio properties, allowing us to study directly the evolution of QSO spectra between redshift z~2 and the present. We find strong evidence for spectral evolution of QSOs. At high redshifts only, we see a new population of radio-quiet QSOs with unusually compact broad-emission-line regions. No significant evolution is seen in the spectra of radio-loud QSOs. We also find that NV (124.0-nm) emission is weaker in radio-loud QSOs, and that the Baldwin effect is stronger in the red wing of CIV than in the blue.en_AU
dc.description.sponsorshipPJF is supported by an ARC grant.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0035-8711en_AU
dc.identifier.urihttp://hdl.handle.net/1885/147258
dc.publisherOxford University Pressen_AU
dc.rightshttp://www.sherpa.ac.uk/romeo/issn/0035-8711/..."author can archive publisher's version/PDF" from SHERPA/RoMEO site (as at 10/09/18)en_AU
dc.sourceMonthly Notices of the Royal Astronomical Societyen_AU
dc.titleThe evolution of QSO spectraen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2en_AU
local.bibliographicCitation.lastpage518en_AU
local.bibliographicCitation.startpage504en_AU
local.contributor.affiliationFrancis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Universityen_AU
local.contributor.authoruidu9710753en_AU
local.description.notesThe author was affiliated with University of Melbourne when the paper was published.en_AU
local.identifier.citationvolume274en_AU
local.identifier.doi10.1093/mnras/274.2.504en_AU
local.publisher.urlhttps://academic.oup.com/journals/en_AU
local.type.statusPublished Versionen_AU

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