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Geometric configuration
for the model. The O VI photons originate from near the hot source (bold
asterisk) and are Raman scattered in the neutral wind (H0-region)
of the cool giant (weakly shaded circle). Grey scales and dotted contours
show emissivity on a log scale. The grid of short straight lines illustrates
the induced polarisation direction for directly scattered Raman photons.
Distances on the axis are in units of 1012 cm.
