Fig. 5

Dependence of the color correction factors fc on the relative luminosity for various NS atmosphere models. The fc are obtained using the first fitting procedure. Top panel: dependences for hydrogen and solar H/He mixture with Z = 0.3 Z⊙ models with different surface gravities log g = 14.0 (solid curves), 14.3 (dotted curves) and 14.6 (dashed curves). For clarity, the dependences for hydrogen models are shifted up by +0.2. Bottom panel: variation of fc on chemical compositions: pure hydrogen (upper curve), pure helium (lowest curve), and solar H/He mixture with Z = Z⊙ (solid curves), Z = 0.3 Z⊙ (dotted curves), Z = 0.1 Z⊙ (dashed curves), Z = 0.01 Z⊙ (dot-dashed curves) for low gravity log g = 14.0 models.
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