Excitation functions of the gamma(o) capture transition in C-12(alpha, gamm
a)O-16 at theta(gamma) = 90 degrees were obtained using a 4 x 4" EGO crysta
l in close geometry (E = 0.94 to 3.39 MeV) and a 2 x 2" EGO crystal in far
geometry (E = 1.69 to 3.29 MeV), where the study of the reaction was initia
ted in inverse kinematics involving a windowless gas target. The small crys
tal detected essentially the E1 multipole component in the gamma(o) capture
transition, while the large crystal observed approximately the angle-integ
rated sum of the E1 and E2 multipole components. Analysis of the two data s
ets together with data from previous work provided strong evidence that bot
h multipoles are of equal importance at the relevant stellar energy E-o = 0
.3 MeV.