  We study static, spherically symmetric black hole solutions in
four-dimensional N=2 gauged supergravity with one vector multiplet and one
hyper-tensor multiplet. This is derived from massive type IIA theory
compactified on the nearly-Kahler coset space G2/SU(3). It is well-known that
the Romans' mass parameter yields the Stuckelberg-type deformation of the gauge
field strengths in the four-dimensional system. This deformation requires that
all the (covariant) derivatives of the scalar fields must vanish and the
two-form field is closed. It turns out that charged solutions are forbidden.
This implies that only AdS vacua or Schwarzschild-AdS black holes are allowed
as the static, spherically symmetric solutions.
