  It has been suggested that the QPO phenomenon in LMXB's could be explained
when the central compact object is a strange star. In this work we investigate
within a standard model for disk accretion whether the observed clustering of
spin frequencies in a narrow band is in accordance with this hypothesis. We
show that frequency clustering occurs for accreting strange stars when typical
values of the parameters of magnetic field initial strength and decay time,
accretion rate are chosen. In contrast to hybrid star accretion no mass
clustering effect is found.
