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Fig. 23


Hertzsprung–Russell diagram showing the position of LHA 120-S 35. The evolutionary tracks for a rotating massive star with 20 M and 25 M taken from Ekström et al. (2012) are plotted in green, from which we obtained by interpolation the evolutionary track for a star with 22 M (in grey). These tracks correspond to solar metallicity Z = 0.014. An isochrone of log t = 7.0 is shown in red.

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