  We present the first numerical results on the binary coalescence of a quark
star with a black hole, obtained with a 3-D Newtonian smooth particle hydro
(SPH) code. The star is initially represented by 17,000 particles modeling a
self-gravitating fluid with the equation of state P= (rho - rho0)c**2/3, and
the black hole by a point mass with an absorbing boundary at the Schwarzschild
radius. As in similar calculations carried out for a stiff polytrope, the
stellar core survives the initial episode of mass transfer, but here an
accretion disk is clearly formed as well.
