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Fig. 11.


Evolution tracks of stellar models of OGLE-LMC-ECL-26122. Thick lines denote the primary models. Error bars indicate the uncertainty in R and Teff reported by Pietrzyński et al. (2013). The models have 0.005 ≤ fos ≤ 0.020 and −0.50 ≤ [Fe/H] ≤ −0.15 (red curves show models with the lowest fos and [Fe/H]).

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