  The cross sections of the 8Li(n,gamma)9Li and 8B(p,gamma)9C capture reactions
have been analyzed using the direct capture model. At low energies which is the
astrophysically relevant region the capture process is dominated by E1
transitions from incoming s-waves to bound p-states. The cross sections of both
mirror reactions can be described simultaneously with consistent potential
parameters, whereas previous calculations have overestimated the capture cross
sections significantly. However, the parameters of the potential have to be
chosen very carefully because the calculated cross section of the
8Li(n,gamma)9Li reaction depends sensitively on the potential strength.
