Be stars are a class of rapidly rotating B stars with circumstellar disks that cause Balmer and other line emission. There are three possible reasons for the rapid rotation of Be stars: they may have been born as rapid rotators, spun up by binary mass transfer, or spun up during the main-sequence (MS) evolution of B stars. To test the various formation scenarios, we have conducted a photometric survey of 55 open clusters in the southern sky. Of these, five clusters are probably not physically associated groups and our results for two other clusters are not reliable, but we identify 52 definite Be stars and an additional 129 Be candidates in the remaining clusters.

Cone search capability for table J/ApJS/161/118/table1 (Photometry of selected stars in open clusters)

Cone search capability for table J/ApJS/161/118/table2 (Summary of open clusters)

Cone search capability for table J/ApJS/161/118/table4 (Distribution of open clusters)