Fluorine production in He-burning regions of massive stars during cosmic history

Open Access

Fig. 4.

Evolution of the surface abundances of the number ratio ¹⁹F to ²²Ne as a function of the number ratio ¹²C to ⁴He for different initial mass stars at super-solar metallicity. The left panel shows the results from non-rotating models, while the right panel shows the results of moderately rotating models.

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