Published August 10, 2016
| Version v1
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Short Period Eclipsing Binaries in the Field of the Young Cluster NGC 2362
Creators
- 1. Dickinson College
- 2. CTIO
- 3. CfA/Harvard
Contributors
Contact person:
Data collector:
Other:
Researchers:
- 1. Dickinson College
- 2. CTIO
- 3. CfA/Harvard
Description
In a study of rotation periods in the young (t ~ 5 Myr) cluster NGC 2362 (Hamilton et al. 2009), several new eclipsing systems were discovered. In this poster, we present photometric observations of these systems and separate them into likely eclipsing binaries and interesting puzzles. The binaries are most likely field stars and are not a part of the cluster.
Notes
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CS19_NGC2362_v4.pdf
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Additional details
References
- Choi, J., et al., 2016, ApJ, 823, 102.
- Hamilton, C. M., et al., 2009, ASP Conference Proceeding, No. 1094, p. 361-364, 2009.