Coulomb dissociation provides an alternative method for determining th
e radiative capture cross sections at astrophysically relevant low rel
ative energies. For the break-up of B-8 on Ni-58, we calculate the tot
al Coulomb dissociation cross section and the angular distribution for
E1, E2 and M1. Our calculations are performed first within the standa
rd first-order semiclassical theory of Coulomb excitation, including t
he correct three-body kinematics, and later including the projectile-t
arget nuclear interactions. We study the dependence of the Coulomb dis
sociation cross section on the structure models assumed for the projec
tile. A range of potential models for Be-7 + p are compared: we look a
t the effect of potential shapes, deformation and inclusion of inelast
ic channels in the projectile states. We analyse the relative Fl and E
2 components and investigate the relation between the measured cross s
ection and the S-factor S-17 Preliminary Coulomb-nuclear interference
results are presented.