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Fig. 8
Teff– log g diagram of our sample stars compared to results in the LMC for early B-type dwarfs from H07 (Hunter et al. 2007) and D18 (Dufton et al. 2018) and for late O-type dwarfs from RG12 (Rivero González et al. 2012) and SS17 (Sabín-Sanjulián et al. 2017).
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