  We review the evidence for AGN optical and X-ray broad line emission from an
accretion disk. We argue that there is little, if any, statistical evidence to
support this assertion. The inconsistency is strongest for the rare class of
Balmer profiles that show double peaks. The line profiles predicted by a simple
illuminated disk model are often incompatible with the observations. We suggest
that the Fe Kalpha line in Seyfert 1 galaxies, where a broad line is most often
and most strongly detected, is actually a composite of two lines both with
Gaussian profiles; one narrow/unshifted and the other broad/redshifted.
