Fig. 2.
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Colour-magnitude diagram of Gaia EDR3 absolute magnitude G and dereddened colour GBP − GRP comparing the observed stars with Ekström et al. (2012) evolutionary tracks without rotation at metallicity Z = 0.014 for stellar masses between 2.5 M⊙ and 6.0 M⊙. Error bars represent the uncertainty on Gabs, corresponding to 3σ error on parallax. The colour index indicates our derived [Fe/H] of the stars.
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