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Fig. 10.

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Absolute G−band magnitudes vs. log α0. The markers are color coded as a function of log Teff. The designation for the α Cygni variables and for stars susceptible to TESS contamination follows that in Fig. 6. We show the linear fit to BSGs with MG fainter than –6.4 mag (thick solid line). The fit (+offset) to the respective parameters of BSGs in the LMC is displayed (dashed line; Bowman et al. 2019a).

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