We model the ~1-200 keV spectra of Cygnus X-3 observed by BeppoSAX. The
continuum, modeled by Comptonization in a hybrid plasma, is modified by the
strongly ionized plasma of the stellar wind of the Wolf-Rayet companion star.
Discrete absorption and emission spectral features are modeled with XSTAR. The
model has been applied to phase-resolved spectra in the hard and soft spectral
states.Comment: 3 pages, to appear in the Proceedings of the Conference "X-ray
Diagnostics of Astrophysical Plasmas", Cambridge, November 15-17, 2004.
Replacement: minor changes in text and acknowledgement
