A study of Be stars in the Magellanic Clouds
  We present the results of a photometric survey for Be stars in eleven young
clusters in the Large Magellanic Cloud and fourteen young clusters in the Small
Magellanic Cloud. B stars with hydrogen in emission are identified on the basis
of their R-H{\alpha} colour. We find that Be star fraction in clusters
decreases with cluster age, and also decreases with the metallicity.
