  We extend our previous study of radiative ablation of circumstellar disks by
line-scattering of the star's radiation, accounting now for the effect of
multiple line resonances off the stellar limb. For an analytic,
three-dimensional model of the velocity structure of an equatorial Keplerian
disk bounded at higher latitudes by a radially accelerating stellar wind
outflow, we use root-finding methods to identify multiple resonances from a
near-disk circumstellar location along starward rays both on and off the
stellar core. Compared to our previous study that accounted only for the effect
of on-core resonances in reducing the radiative driving through the scattering
of radiation away from a near-disk circumstellar location, including off-limb
resonances leads to additional radiative driving from scattering toward this
location. Instead of the up-to-50% reduction in line-acceleration previously
inferred from multiple resonance effects, we now find a more modest 15-20% net
reduction.
