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Fig. 10

image

Absorption-corrected 210 keV X-ray flux versus nuclear UV flux estimated from models. The symbols indicate the median value for the estimated UV luminosities from their respective best-fit models, and the lines indicate the dispersion (68% area) in the possible values. Type I galaxies that can only be fit with type A models (filling factors 0.41.4%) are given as filled circles. Those that can also be fit by type B models (filling factors 5.320%) are shown twice, with the model UV-flux values given as triangles (model A) and asterisks (model B). All type 2 galaxies are shown as asterisks.

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