X-ray studies of quasars with the Einstein Observatory. II

G. Zamorani, J. P. Henry, T. Maccacaro, H. Tananbaum, A. Sołtan, Y. Avni, James Liebert, John T. Stocke, P. A. Strittmatter, R. J. Weymann,

The Astrophysical Journal · 1981 · 387 citations · 0 references

Concepts

Abstract

X-ray observations of 107 quasars have been carried out with the Einstein Observatory, and 79 have been detected. A correlation between optical emission and X-ray emission is found; and for radio-loud quasars, the data show a correlation between radio emission and X-ray emission. For a given optical luminosity, the average X-ray emission of radio-loud quasars is about three times higher than that of radio-quiet quasars. The data also suggest that the ratio of X-ray to optical luminosity is decreasing with increasing redshift and/or optical luminosity. The data support the picture in which luminosity evolution, rather than pure density evolution, describes the quasar behavior as a function of redshift.