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Published online by Cambridge University Press: 19 July 2016
We 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.
3: Further Reading
See Francis, Hooper & Impey, 1993, Astronomical Journal 106, 417 and references therein for more details and discussion.