  We present new results obtained with the VLT GIRAFFE for a large sample of B
and Be stars belonging to the Magellanic Clouds, i.e. at low metallicity.
First, we show the effects of the metallicity of the environment on their
rotation (linear, angular, and at the ZAMS). Second, we present the analysis of
the effects of metallicity and evolution on the appearance of Be stars. We also
new present results about the proportions of Be stars to B stars. Third, by
cross-correlation with large photometric surveys such as MACHO and OGLE, we
report on the detection for the first time of short-term multi-periodicity in 9
Be stars in the Small Magellanic Cloud, which can be interpreted in terms of
pulsations.
