Be stars in and around young clusters in the Magellanic Clouds
We present the results of a search for Be stars in six fields centered on the young clusters NGC 330 and NGC 346 in the SMC, and NGC 1818, NGC 1948, NGC 2004 and NGC 2100 in the LMC. Be stars were identified by differencing R band and narrow-band Hα CCD images. Our comparatively large images provide substantial Be star populations both within the clusters and in their surrounding fields. Magnitudes, positions and finding charts are given for the 224 Be stars found. The fraction of Be stars to...[Show more]
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics Supplement Series|
|Be_stars.pdf||1.32 MB||Adobe PDF|
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