  We report the discovery with BeppoSAX-WFC of two new X-ray sources that were
only seen during bursts: SAX J1753.5-2349 and SAX J1806.5-2215. For both
sources, no steady emission was detected above an upper limit of 5 mCrab (2 to
8 keV) for 3 10**5 s around the burst events. The single burst detected from
SAX J1753.5-2349 shows spectral softening and a black body color temperature of
2.0 keV. Following the analogy with bursts in other sources the burst very
likely originates in a thermonuclear flash on a neutron star. The first of two
burst detected from SAX J1806.5-2215 does not show spectral softening and
cannot be confirmed as a thermonuclear flash.
