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The cosmic origin of fluorine is still under debate. Asymptotic giant branch(AGB) stars are among the few suggested candidates to efficiently synthesis Fin our Galaxy, however their relative contribution is not clear. In this paper,we briefly review the theoretical studies from stellar yield models of the Fsynthesis and chemical equilibrium models of the F-containing molecules in theoutflow around AGB stars. Previous detections of the F-bearing species towardsAGB and post-AGB stars are also highlighted. We suggest that high-resolutionALMA observations of the AlF, one of the two main carriers of F in the outflowof AGB stars, can provide a reliable tracer of the F-budget in AGB stars. Thiswill be helpful to quantify the role of AGB stars in the Galactic F budget.

Tracing the role of AGB stars in the Galactic Fluorine budget