On the Apsidal Motion of IQ Persei
CCD observations of times of minimum light of IQ Per with apsidal motion were made in VR bandpasses for four nights from November to December, 2002. From the observations four times of minimum light were determined. All times of minimum light collected from literatures, including ours, were analyzed...
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Korean Space Science Society (KSSS)
2003-12-01
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doaj-5ac551ce8c7042ae9026b2a3cb0c229c2020-11-25T00:03:23ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14092003-12-0120426126810.5140/JASS.2003.20.4.261On the Apsidal Motion of IQ PerseiChung-Uk Lee0Chun-Hwey Kim1Kyu-Dong Oh2Yong-Ik Byun3Korea Astronomy Observatory, Daejeon 305-348, KoreaDept. of Astronomy & Space Science, College of Natural Science and Institute for Basic Science Research, Chungbuk National University, Cheongju 361-763, KoreaDept. of Earth Science Education, Chonnam National University, Kwangju 500-757, KoreaDepartment of Astronomy and Space Science, Yonsei University, Seoul, 120-749, KoreaCCD observations of times of minimum light of IQ Per with apsidal motion were made in VR bandpasses for four nights from November to December, 2002. From the observations four times of minimum light were determined. All times of minimum light collected from literatures, including ours, were analyzed to determine the apsidal motion parameters of IQ per. The sidereal and apsidal motion periods were calculated to be 0.035 s and 0.2 y slightly longer than those of Değirmenci (1997), respectively. The apsidal motion parameters of IQ Per derived in this paper show good agreement with Değirmenci's values. Our results support his internal density constant of bar{k}2obs = 0.0038 for IQ Per and 5 % accuracy of agreement between the observed and modelled values of the apsidal motion constant.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2003/v20n4/OJOOBS_2003_v20n4_261.pdfeclipsing binaryIQ Pertimes of minimum lightapsidal motion |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Chung-Uk Lee Chun-Hwey Kim Kyu-Dong Oh Yong-Ik Byun |
spellingShingle |
Chung-Uk Lee Chun-Hwey Kim Kyu-Dong Oh Yong-Ik Byun On the Apsidal Motion of IQ Persei Journal of Astronomy and Space Sciences eclipsing binary IQ Per times of minimum light apsidal motion |
author_facet |
Chung-Uk Lee Chun-Hwey Kim Kyu-Dong Oh Yong-Ik Byun |
author_sort |
Chung-Uk Lee |
title |
On the Apsidal Motion of IQ Persei |
title_short |
On the Apsidal Motion of IQ Persei |
title_full |
On the Apsidal Motion of IQ Persei |
title_fullStr |
On the Apsidal Motion of IQ Persei |
title_full_unstemmed |
On the Apsidal Motion of IQ Persei |
title_sort |
on the apsidal motion of iq persei |
publisher |
Korean Space Science Society (KSSS) |
series |
Journal of Astronomy and Space Sciences |
issn |
2093-5587 2093-1409 |
publishDate |
2003-12-01 |
description |
CCD observations of times of minimum light of IQ Per with apsidal motion were made in VR bandpasses for four nights from November to December, 2002. From the observations four times of minimum light were determined. All times of minimum light collected from literatures, including ours, were analyzed to determine the apsidal motion parameters of IQ per. The sidereal and apsidal motion periods were calculated to be 0.035 s and 0.2 y slightly longer than those of Değirmenci (1997), respectively. The apsidal motion parameters of IQ Per derived in this paper show good agreement with Değirmenci's values. Our results support his internal density constant of bar{k}2obs = 0.0038 for IQ Per and 5 % accuracy of agreement between the observed and modelled values of the apsidal motion constant. |
topic |
eclipsing binary IQ Per times of minimum light apsidal motion |
url |
http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2003/v20n4/OJOOBS_2003_v20n4_261.pdf |
work_keys_str_mv |
AT chunguklee ontheapsidalmotionofiqpersei AT chunhweykim ontheapsidalmotionofiqpersei AT kyudongoh ontheapsidalmotionofiqpersei AT yongikbyun ontheapsidalmotionofiqpersei |
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