Fig. 11

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Global AMR of the Magellanic Bridge found using the PADOVA-COLIBRI (red line) and BaSTI (blue line) stellar models. The left portion of the abscissa is in logarithmic scale to better appreciate the details, while the right portion is in linear scale. The shaded area represents the confidence interval of our solution, computed as the fifth and 95th percentiles of the parameters’ distribution. The dashed green line marks the global AMR of the SMC obtained by Rubele et al. (2018), while the dashed black line represents the AMR of the LMC from Carrera et al. (2008b).
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