Relativistic beaming and the optical magnitudes of QSOs

Details Relativistic beaming and the optical magnitudes of QSOs Relativistic beaming and the optical magnitudes of QSOs

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213...97b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, March 1, 1985, p. 97-102.

Astronomy and Astrophysics

Astronomy

36

Magnitude, Optical Properties, Quasars, Radio Spectra, Very Long Base Interferometry, Flux Density, Histograms, Visual Observation

Scientific paper

The authors have compared the optical magnitudes of weak, lobe-dominated QSOs and strong, core-dominated QSOs. They find differences in the average magnitudes of the two classes of objects which imply at least one magnitude of enhancement of the optical continuum radiation in core-dominated sources if the Orr & Browne unified scheme of QSOs is correct. Some further observational tests of the scheme are suggested.

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