Figure 1 from Convective Overshoot Mixing in Models of the Stellar Interior

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Convective Overshoot Mixing in Models of the Stellar Interior

Authors: Q. S. Zhang

Zhang 2013 The Astrophysical Journal Supplement Series 205 18.

Provider: AAS Journals

Caption: Figure 1.

Sound speed differences in the solar models. is the sound speed difference. c _model is the sound speed of the model. c _☉ is the helioseismic inversion of sound speed taken from Basu et al. (2009).

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