The reactions and ashes of thermonuclear explosions on neutron stars
  This paper reports on the detailed rp-process reaction flow on an accreting neutron star and the resulting ashes of a type I X-ray burst. It is obtained by coupling a 298 isotope reaction network to a self-consistent one-dimensional model calculation with a constant accretion rate of dM/dt=1.0e17g/s (0.09 Eddington). 
J.L. Fisker, E. Brown, M. Liebendoerfer, F.-K. Thielemann, and M.   Wiescher