  A star surrounded by a black hole generated by it is analyzed. For an outer
static observer the black hole mass (and radius) depends on his position in the
gravitational field of the star. In spite of the black hole presence, the
geometry remains that of Schwarzschild. For an inner observer the black hole
mass is constant and depends on the star's mass $m$ and radius $R$. The entropy
for $r > R$ is one quarter of the area and is constant for $r < R$.
