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Optical Differences Between Radio-Loud and Radio-Quiet QSOs

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dc.contributor.authorFrancis, Paul
dc.date.accessioned2018-10-03T02:56:15Z
dc.date.available2018-10-03T02:56:15Z
dc.date.issued1994
dc.description.abstractWe analyse the rest-frame UV spectra of a complete sample of optically selected radio-loud and radio-quiet QSOs. Our results are: 1: Broad absorption-line QSOs (BALQSOs) are all radio quiet, but they are strongly clustered toward the top end of the radio-quiet population in radio power. 2: Radio-loud QSOs have higher equivalent-width, narrower high ionisation emission-lines than radio-quiet QSOs.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.urihttp://hdl.handle.net/1885/148061
dc.publisherInternational Astronomical Unionen_AU
dc.relation.ispartofMulti-wavelength continuum emission of AGN: proceedings of the 159th Symposium of the International Astronomical Union; held in Geneva; Switzerland; August 30-September 3; 1993en_AU
dc.rights© International Astronomical Unionen_AU
dc.source.urihttp://adsabs.harvard.edu/abs/1994IAUS..159..503Fen_AU
dc.titleOptical Differences Between Radio-Loud and Radio-Quiet QSOsen_AU
dc.typeConference paperen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.startpage503en_AU
local.contributor.affiliationFrancis, P., Mount Stromlo Observatory, Research School of Astronomy and Astrophysics, The Australian National Universityen_AU
local.contributor.authoruidu9710753en_AU
local.type.statusPublished Versionen_AU

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