The magneto-rotational instability in massive stars

Open Access

Fig. 5.

Impact of MRI and the TS dynamo on chemical transport during the MS. Left panel: same as the right panel of Fig. 3 but comparing our reference models to those where the TS dynamo is included. Right panel: same as in Fig. 2b but for the models discussed in Sect. 4.3 (see plot legends).

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