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

Open Access

Fig. 7.

Comparisons between the wind stellar yields of ¹⁹F in units of 10⁻⁶ M_⊙ obtained by this work (purple curves) from models by Ekström et al. (2012) and by Palacios et al. (2005b) (black curves) with the same stellar evolution code for solar metallicities.

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