  We propose that the scatter in line width versus luminosity of the BLR of AGN
arises from a dependence on the line of sight to an axially symmetric BLR.
Adopting a simple model for the line width as a function of luminosity and
angle, and convolving this with the observed luminosity function, allows us to
predict a line width distribution consistent with the available data.
Furthermore, we use the relation between the equivalent width of a line and the
luminosity in the continuum to predict an observed correlation between line
width and equivalent width. The scatter on this correlation is again provided
by angular dependence. We also show a viewing angle dependence can produce the
X-ray spectral index distribution. The results have applications as diagnostics
of models of the broad line region and in cosmology.
