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. 2017 Aug 23;4(8):170192. doi: 10.1098/rsos.170192

Figure 13.

Figure 13.

Location of the mass boundaries as a function of time (zero point taken at the completion of the first dredge-up) of the convective envelope, H-burning shell and the zone mixed by the thermohaline instability, for a low-mass RGB stellar model.