  The motions of comets and neutron stars have been integrated over five
billion years in the Galactic potential to determine a gamma-ray burst
distribution, presuming that bursts are the result of interactions between
these two families of objects. The comets originate in two distinct populations
- one from ejection by stars in the Galactic disk, and the other from ejection
by stars in globular clusters. No choice of the free parameters resulted in
agreement with both the isotropy data and the $\log(N>F) - \log(F)$ data.
