| Deep Infrared Imaging of the R Corona Australis Cloud Core (2007) | |||||||||||||||
Abstract | |||||||||||||||
| Preliminary analysis is presented for J, H, and K 0 images of the Corona Australis cloud core. Color-color and color-magnitude diagrams reveal relatively few new cluster members. We conclude that the R Cr A infrared cluster consists of only about 30 members and its size reflects the available reservoir of molecular gas. Subject headings: star formation-- R Coronae Australis-- 3-- | |||||||||||||||
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