Grids of stellar models with rotation - VIII. Models from 1.7 to 500 M⊙ at metallicity Z = 10−5

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Fig. 1.

Evolutionary tracks in the HRD for non-rotating (left) and rotating (right) models, colour-coded according to the surface number abundance of nitrogen log(N/H [numb.]) + 12. Each track is labelled with its initial mass. Every other star below 9 M_⊙ is shown with a dashed line in order to better distinguish the models.

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