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We report the results of the observations of the three gamma-ray pulsars PSRB0656+14, PSR B1055-52 and PSR B1706-44 performed with BeppoSAX. We detected apulsed emission only for PSR B1055-52: in the range 0.1-6.5 keV the pulseprofile is sinusoidal and the statistical significance is 4.5 sigma. The pulsedfraction was estimated 0.64+/-0.17. This pulsation was detected also atenergies greater than 2.5 keV suggesting either a non-thermal origin or a quitehigh temperature region on the neutron star surface. Spectral analysis showedthat only the X-ray spectrum of PSR B1706-44 can be fitted by a singlepower-law component, while that of PSR B1055-52 requires also a blackbodycomponent (kT = 0.075 keV) and that of PSR B0656+14 two blackbody components(kT_1 = 0.059, kT_2 = 0.12 keV).Comment: 8 pages, 5 figures. Accepted for publication in A&

BeppoSAX observations of the three Gamma-ray pulsars PSR B0656+14, PSR B1055-52 and PSR B1706-44