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Fig. 4
Comparison of the observed (IUE observations: filled circles, uvby photometry unreddened by E(b − v) = 0.12: open circles), and modeled SED for HD 50975. The solid line represents a composite SED of two stars of spectral type F8 Iab and B1 V with a ratio of fluxes of 0.12 at 5500 Å.
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