Preliminary results on BeppoSAX LEGS and MECS observations of BL Lacer
tae objects selected from the 1 Jy sample are presented. All sources o
f the LBL type, that is, characterized by a peak in their multifrequen
cy spectra at infrared/optical energies, seem to show a relatively fla
t (alpha(x) similar to 0.7 - 0.8) X-ray spectrum. This is in agreement
with the supposed dominance of inverse Compton emission in the X-ray
band of these sources.