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We present BeppoSAX observations of the two FR I type radio galaxies HerculesA (3C 348) and MRC 0625-536 in the energy range $0.2 - 200$ keV. Data analysisshows that the X-ray flux from Hercules A is consistent with a diffuse thermalplasma emitting at $T \approx 4-5$ keV with a possible, but somewhat uncertain,contribution of a softer component at $T \approx 3 $ keV. The non thermalemission from the active nucleus must be significantly smaller than the thermalone, and no indication of relevant core obscuration by a surrounding torus wasdetected. The flux from MRC 0625-536 originates form an extended region and hasbeen fitted to a thermal law with $T \approx 5.7$ keV and with a column densityconsistent with the galactic absorption. A spatially resolved spectral analysisdoes not show a relevant variation of the temperature and the metallicityacross the diffuse emission zone. A non thermal spectral component, related tothe nuclear activity, may be present in the innermost region with some possibleamount of local obscuration, contributing $\lapp 10%$ to the total luminosity.Hard X-ray emission from MRC 0625-536 has been detected in the PDS (15 - 200keV) that may be related either to its galactic core or to the intraclusterregion.Comment: 8 pages, 3 figures; to appear in Astronomy & Astrophysic

BeppoSAX observation of Hercules A and MRC 0625-536