Fig. 9
Comparison of our Teff calibration for O dwarfs in the LMC with those derived by Rivero González et al. (2012a,b) and adopted by Doran et al. (2013). Grey dots and bars represent the mean value and standard deviation of our Teff estimates for each spectral type, with our linear fit shown by the black line (and the grey zones indicating the associated uncertainties).
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