The big bump in quasar spectra

Details The big bump in quasar spectra The big bump in quasar spectra

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.265o&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 265-268 (SEE N89

Astronomy and Astrophysics

Astronomy

Iue, Quasars, Spaceborne Astronomy, Spectral Energy Distribution, Ultraviolet Astronomy, Ultraviolet Spectra, Infrared Astronomy, Radio Astronomy, Stellar Luminosity, X Ray Astronomy

Scientific paper

The relations between the radio, infrared, ultraviolet, and X-ray luminosities for a sample of radio quiet and radio loud quasars are quantified. For both subsamples the relations between the X-ray and the ultraviolet or infrared luminosities are consistent, and are significantly nonlinear. There is a linear relation between the infrared and ultraviolet luminosities. For the quasars for which Log L(1450) greater than or = 29.5 or Log L(1 mn) greater than or = 30.5 there is no correlation between the strength of the big bump and luminosity.

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