Key points are not available for this paper at this time.
Black hole mergers with neutron stars are promising sources of gravitational-wave signals for the new crop of gravitational wave detectors. The impressive numerical relativity simulations carried out in this paper illustrate what to expect when the orientation of the black hole spin and the equation of state of the neutron star are properly taken into account.
Kawaguchi et al. (Tue,) studied this question.