  We introduce our VLT-FLAMES survey of massive stars in the Galaxy and the
Magellanic Clouds, giving details of the observations in our younger fields in
the LMC and SMC. In particular we highlight a new O2.5-type star discovered in
N11, and Be-type stars in NGC 346 with permitted Fe II emission lines in their
spectra. We give an overview of the distribution of spectral types in these
fields and summarize the observed binary fraction.
