The Leavitt law on multi-phase discussion

碩士 === 國立中央大學 === 天文研究所 === 99 === We use the Optical Gravitational Lensing Experiment III (OGLE III) classical Cepheid data to derive multi-phase period-luminosity relation ( PL relation), and compare with mean PL relation in the application of distance estimator. First, we discuss the difference...

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Main Authors: Ya-hong Lin, 林雅紅
Other Authors: Chow-Choong Ngeow
Format: Others
Language:zh-TW
Published: 2011
Online Access:http://ndltd.ncl.edu.tw/handle/58869289522664866905
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spelling ndltd-TW-099NCU051990052017-07-06T04:42:56Z http://ndltd.ncl.edu.tw/handle/58869289522664866905 The Leavitt law on multi-phase discussion 以多相位的角度探討萊維特定律 Ya-hong Lin 林雅紅 碩士 國立中央大學 天文研究所 99 We use the Optical Gravitational Lensing Experiment III (OGLE III) classical Cepheid data to derive multi-phase period-luminosity relation ( PL relation), and compare with mean PL relation in the application of distance estimator. First, we discuss the difference in PL relation''s dispersion. It exists that there''s a phase with smaller dispersion value than mean''s, but thier difference is small. In addition, there is a bump existed in a specific phase, it might be due to Cepheid pulsational inner shock. We also performed self-testing in estimating distance using different observational data in LMC''s Cepheids. The distance derived from multi-phase PL relations is closer than the distance derived from mean PL relation, and they are reasonable because they are within errors. We suggest to test other galaxy''s distance to discuss their differences in more detail. Chow-Choong Ngeow 饒兆聰 2011 學位論文 ; thesis 35 zh-TW
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language zh-TW
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description 碩士 === 國立中央大學 === 天文研究所 === 99 === We use the Optical Gravitational Lensing Experiment III (OGLE III) classical Cepheid data to derive multi-phase period-luminosity relation ( PL relation), and compare with mean PL relation in the application of distance estimator. First, we discuss the difference in PL relation''s dispersion. It exists that there''s a phase with smaller dispersion value than mean''s, but thier difference is small. In addition, there is a bump existed in a specific phase, it might be due to Cepheid pulsational inner shock. We also performed self-testing in estimating distance using different observational data in LMC''s Cepheids. The distance derived from multi-phase PL relations is closer than the distance derived from mean PL relation, and they are reasonable because they are within errors. We suggest to test other galaxy''s distance to discuss their differences in more detail.
author2 Chow-Choong Ngeow
author_facet Chow-Choong Ngeow
Ya-hong Lin
林雅紅
author Ya-hong Lin
林雅紅
spellingShingle Ya-hong Lin
林雅紅
The Leavitt law on multi-phase discussion
author_sort Ya-hong Lin
title The Leavitt law on multi-phase discussion
title_short The Leavitt law on multi-phase discussion
title_full The Leavitt law on multi-phase discussion
title_fullStr The Leavitt law on multi-phase discussion
title_full_unstemmed The Leavitt law on multi-phase discussion
title_sort leavitt law on multi-phase discussion
publishDate 2011
url http://ndltd.ncl.edu.tw/handle/58869289522664866905
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