Fig. 11
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Comparison of teff_esphs with the effective temperature expected from the spectral type and the effective temperature given in GES. Left panel: effective temperature from spectral types versus the Gaia DR3 effective temperature teff_esphs for the Car OB1 high-mass star sample. The stars highlighted in magenta have spectraltype_esphs O. Right panel: Gaia DR3 effective temperature teff_esphs versus effective temperature from GES for stars in the region of Car OB1.
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