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Fig. 14


Emergent Eddington flux Hν versus wavelength calculated for very massive 3000 M stars with effective temperature 65 000 K and radius 79 R, for different compositions (a metallicity of 1.0 and 0.05 Z and a hydrogen mass fraction of 0.7 (first row), and a metallicity of 1.0 Z and a hydrogen mass fraction of 0.4 (second row)), compared to an equivalent blackbody.

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