After calibrating the neutrino-process yields to the observed 11B/10B ratio, the model predicts that AGB stars, not the neutrino process, supply most of the present-day fluorine in the galaxy.
@doi [ ] 10.1051/0004-6361/201118623, https://ui.adsabs.harvard.edu/abs/2012A&A...540A...3A 540
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Constraining $\nu$-Process Production of Fluorine through Cosmic Ray Nucleosynthesis
After calibrating the neutrino-process yields to the observed 11B/10B ratio, the model predicts that AGB stars, not the neutrino process, supply most of the present-day fluorine in the galaxy.