Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
碩士 === 國立中央大學 === 天文研究所 === 99 === Time-series photometric observations were carried over sixty nights in 2009 using the 81-cm Tenagra telescope in Arizona within the framework of a multi-year survey program of variable stars in open clusters. The analysis of NGC 1513 and NGC 225 was a pilot study o...
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2011
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| Online Access: | http://ndltd.ncl.edu.tw/handle/82040872684550253495 |
| Summary: | 碩士 === 國立中央大學 === 天文研究所 === 99 === Time-series photometric observations were carried over sixty nights in 2009
using the 81-cm Tenagra telescope in Arizona within the framework of a multi-year
survey program of variable stars in open clusters. The analysis of NGC 1513 and
NGC 225 was a pilot study of this effort, we also developed the basic algorithms
of the eclipsing binary to compute the data points from our observations to
understand the characteristics of eclipsing binary stars in NGC 1513 and NGC
225. About the model, we create some invented observation data to prove the
accuracy of its. Totally we find the 12 variable stars including 6 eclipsing
binaries in NGC 1513 and NGC 225 and get the results of the model fitting of
eclipsing binaries.
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