  Several resonances in the $^{15}$N($\alpha$,$\gamma$)$^{19}$F reaction have
been investigated in the energy range between 0.6 MeV and 2.7 MeV. Resonance
strengths and branching ratios have been determined. High sensitivity could be
obtained by the combination of the {\sc{dynamitron}} high current accelerator,
the windowless gas target system {\sc{rhinoceros}}, and actively shielded
germanium detectors. Two levels of $^{19}$F could be observed for the first
time in the ($\alpha$,$\gamma$) channel, and several weak branchings below the
detection limits of previous experiments were measured. Two observed resonances
correspond to $\alpha$-cluster states in $^{19}$F which have been assigned
unambiguously. The astrophysical reaction rate is derived from this set of
resonance strengths.
