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| Paper: |
IRAS 20050+2720: Anatomy of a Young Stellar Cluster |
| Volume: |
448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun |
| Page: |
625 |
| Authors: |
Günther, H. M.; Wolk, S. J.; Gutermuth, R. A.; Spitzbart, B.; Bourke, T. L.; Pillitteri, I.; DeRose, K. |
| Abstract: |
We present early results of our multiwavelength study of the star forming region IRAS 20050+2720. While we use X-rays and IR to classify young stellar objects, the optical data can be used to exclude foreground objects. The dataset set contains 57 class I sources, 183 class II sources and 183 X-ray sources, of which 140 are class III candidates. Within IRAS 20050+2720 four subclusters are found. Subcluster A and B are the densest regions, which contain stars of all evolutionary stages. Subcluster C is much younger than the other two. It has not formed any class III objects yet. We newly identify a fourth subcluster, which consists mostly of class II objects and is located about 10′ from the center of the cloud. |
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