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Correlation of X-Ray and Infrared Emission of Radio-Quiet QSOs

Published online by Cambridge University Press:  19 July 2016

D. M. Worrall*
Affiliation:
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, U.S.A.

Abstract

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A correlation of the form , with γ = 0.83, is found between 2 keV monochromatic X-ray luminosity and 1.65 μm monochromatic infrared luminosity for a sample of optically selected radio-quiet QSOs. This is equivalent to an average 1.65 μm to 2 keV spectral index of αir/x = 1.28+0.05 log(lir/1031 ergs s−1 Hz−1). The ratio of X-ray to infrared luminosity decreases with increasing infrared luminosity in a manner similar to the relationship between X-ray and optical luminosity. The standard deviations of the distributions of data about the best-fit functions are comparable for the X-ray versus infrared and X-ray versus optical fits. Thus, contrary to a previous claim, the infrared luminosity is not better than the optical luminosity at predicting the X-ray emission from QSOs.

Type
Chapter X: The Distribution of X-Ray Sources and the X-Ray Background
Copyright
Copyright © Reidel 1987 

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