  Using data from the EROS2 microlensing survey, we report the discovery of two
blue objects with irregular photometric behaviour of $\Delta V \sim 0.1$-0.4
mag on time scales of 20 to 200 days. They show a bluer when fainter behaviour.
Subsequent spectra taken with the ESO 3.6m telescope show spectral type B4eIII
and B2eIV-V with strong $H \alpha$ emission. These objects resemble the Herbig
AeBe but also classical Be stars. At this stage, it is not possible to
distinguish unambiguously between pre-main sequence and classical Be nature. If
we favour the pre-main sequence interpretation, they are more luminous than the
luminosity upper limit for Galactic HAeBe stars. The same was found for the
HAeBe candidates in the LMC. This might be due to a shorter accretion time
scale ($\tau = M_*/\dot{M}$), or the smaller dust content during the pre-main
sequence evolution of SMC and LMC stars.
