Fig. 9
Surface abundances expected for models with turbulence anchored at , Z0 ~ 0.0001 and three slightly different masses, or equivalenty Teff. Observations for star B315 of M 15 with Teff ~ 13 000 K are from Behr (2003). These are the same observations as used in the right panel of Fig. 11 of Michaud et al. (2008). The turbulence models are different, however. The agreement is equivalent.
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