Abstract
We examine the correlations of X-ray and optical luminosities with radio properties for radio-selected quasars. A remarkably strong correlation is found to exist between the total radio luminosity (irrespective of whether it comes from a compact core or extended lobes) and the X-ray luminosity. A weaker correlation is found between the radio luminosity and the optical luminosity. The results are consistent with a two-component origin for the optical/X-ray emission, one isotropic and one relativistically beamed. This model also accounts for the change of slope with radio structure for the radio/X-ray luminosity correlation noted by Kembhavi et al. Quasars with flat radio spectra are found to have smaller emission-line equivalent widths than do steep-spectrum quasars, again in the sense predicted by the beaming hypothesis.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
