Excited states in Ce-126 have been observed with the GAMMASPHERE gamma -ray
detector array, used in conjunction with the MICROBALL charged-particle de
tector. The reaction Zn-64(Zn-64, xpn alpha) (beam energy 260 MeV) was used
to populate a wide range of nuclei in the neutron-deficient region with A
approximate to 120. Ce-126 was populated via the 2p evaporation channel. Th
e three previously observed bands have been extended to higher spins and so
me other structures have been identified. The yrast band shows evidence of
a delayed neutron alignment occurring at a rotational frequency omega appro
ximate to0.5 MeV/(h) over bar as observed in the neighboring odd-A nucleus
Pr-127. One of the two excited bands shows evidence for a similar crossing
at a slightly lower frequency and also exhibits a sudden gain in alignment
at omega =0.57 MeV/(h) over bar. The third band may involve the coupling of
a gamma -vibrational state. All three rotational bands are discussed in te
rms of standard and extended cranked shell model calculations.