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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Main Authors: Ping-Han Cheng, 鄭秉漢
Other Authors: Wing-Huen Ip
Format: Others
Language:zh-TW
Published: 2011
Online Access:http://ndltd.ncl.edu.tw/handle/82040872684550253495
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spelling ndltd-TW-099NCU051990012017-07-06T04:42:56Z http://ndltd.ncl.edu.tw/handle/82040872684550253495 Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225 疏散星團NGC 1513與NGC 225中的食雙星測光分析 Ping-Han Cheng 鄭秉漢 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. Wing-Huen Ip 葉永烜 2011 學位論文 ; thesis 96 zh-TW
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language zh-TW
format Others
sources NDLTD
description 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.
author2 Wing-Huen Ip
author_facet Wing-Huen Ip
Ping-Han Cheng
鄭秉漢
author Ping-Han Cheng
鄭秉漢
spellingShingle Ping-Han Cheng
鄭秉漢
Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
author_sort Ping-Han Cheng
title Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
title_short Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
title_full Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
title_fullStr Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
title_full_unstemmed Photometric Study and Time-Series Analysis of the Open Clusters NGC 1513 and NGC 225
title_sort photometric study and time-series analysis of the open clusters ngc 1513 and ngc 225
publishDate 2011
url http://ndltd.ncl.edu.tw/handle/82040872684550253495
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