We present a BeppoSAX survey of five Be/X-ray binary candidates .
We report on the identification of two of them , HD 110432 and HD 141926 , as low luminosity Be/X-ray binaries .
For HD 110432 we report on the detection of a pulsation period of \sim 14 ks .
Because the luminosity of these sources is low and their spectra do not require non-thermal emission models , these systems are good Be+White Dwarf candidates .
If the pulsation period for HD 110432 is confirmed , this system would be the most firm Be+WD candidate found up to date .
The other three objects HD 65663 , HD 249179 and BD+53 2262 did not show detectable X-ray emission .
We argue that , while the properties of BD+53 2262 are still consistent with a quiescent Be+Neutron Star scenario , the lack of detection for the other two objects implies that they are most probably not X-ray binaries .