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On the profiles and the polarization of Raman-scattered emission lines in symbiotic stars -- II. Numerical simulations
A Monte Carlo method is used to calculate the profiles and the polarization of the Raman-scattered O vi lines (λλ6827, 7088) in symbiotic stars, which are believed to consist of a binary system of a cool giant and a hot star with an emission nebula around it. A point-like isotropic …