Fig. 5
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Gaia Gmag versus distance (from Bailer-Jones et al. 2021) for stars located within H II regions listed in Table 2. Blue dots correspond to spectral types earlier than B2, and pink dots to spectral types later than B2. Vertical lines show the distance uncertainties. Dashed lines mark the adopted distance limits of 2.2 and 3.2 kpc.
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