Previous studies of 172Os noted an anomaly in the behaviour of the mom
ent of inertia of the yrast band at low spin. A phenomenological model
of shape coexistence based on interacting rotational bands was propos
ed to explain this anomaly and this model predicted low-lying non-yras
t states. In order to test these predictions, the beta-decay of 172Ir
has been used to populate 172Os. Excited states have been observed and
classified into positive-parity ''quasi-beta'' and ''quasi-gamma'' ba
nds and a negative-parity band. The energies of the quasi-beta band st
ates are seen to be in general agreement with the predictions of the p
henomenological model and the model is refined to take into account th
e new data. The bands involved are determined to have significantly di
fferent moments of inertia.