Open Access

Fig. 6.


Best fit massive-star models for the CEMP-no star ET0097 at [Fe/H] = −2. Points with errorbars are 1D LTE abundance measurements from Skúladóttir et al. (2015a). Three models are shown with lines, computed at three different initial rotational velocities, υini/υcrit = 0 (black), 0.4 (red) and 0.7 (blue). All models are for 25 M stars at Z = 10−3. The reduced χ2 of each fit are shown on the top right, and the residuals of the fits are in the bottom panel.

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