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