Stellar models and isochrones from low-mass to massive stars including pre-main sequence phase with accretion

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Fig. 11.

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Comparison between the isochrones of 10⁶ yr, 10^6.5 yr and 10⁷ yr of the grid and observations of the IC 1848 and NGC 1893 clusters, from Lim et al. (2014a,b).

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