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Fig. 3


a) Temperature stratifications for two different PPM (blue line) and SphM (red line) stellar models with effective temperature of Teff = 5000 K and log g = 4.5. b) Stratification of normalized absorption (solid line) and scattering (dashed line) opacities for PPM (blue) and SphM (red) of the stellar atmospheres with Teff = 5000 K. c) Center-to-limb variation of intensity for PPM (blue line) and SphM (red line). d) Center-to-limb variation of polarization for PPM (blue line) and SphM (red line). The panels e)h) show the same values as in a)d), but for stellar models with Teff = 6500 K and the same value of surface gravity, respectively.

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