  We review all the BeppoSAX results relative to the search for additional
nonthermal components in the spectra of clusters of galaxies. In particular,
our MECS data analysis of A2199 does not confirm the presence of the nonthermal
excess reported by Kaastra et al. (1999). A new observation of A2256 seems to
indicate quite definitely that the nonthermal fluxes detected in Coma and A2256
are due to a diffuse nonthermal mechanism involving the intracluster medium. We
report marginal evidence (~3\sigma) for a nonthermal excess in A754 and A119,
but the presence of point sources in the field of view of the PDS makes
unlikely a diffuse interpretation.
