Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193..537j&link_type=abstract
Monthly Notices of the Royal Astronomical Society, vol. 193, Nov. 1980, p. 537-548.
Astronomy and Astrophysics
Astronomy
12
Astronomical Spectroscopy, Emission Spectra, Line Spectra, Quasars, Reference Stars, Stellar Spectra, Carbon, Hubble Diagram, Red Shift, Spectral Line Width
Scientific paper
It is difficult to observe emission lines of small equivalent width in intrinsically faint QSOs. This selection effect biasses the slope of the log (intrinsic continuum luminosity) versus log (C-IV equivalent width) diagram for samples of QSOs such as those of Baldwin and those taken from slitless spectrum surveys. There is no such bias for QSO samples drawn from radio surveys, and such data suggest that the total flux of the C IV line may itself be a good standard candle. The best way to determine q(0) from QSO samples may be to look at the upper envelope of the m(C-IV)-Z relationship.
Jones Bernard J. T.
Jones Janet E.
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