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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Main Authors: Chung-Uk Lee, Chun-Hwey Kim, Kyu-Dong Oh, Yong-Ik Byun
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 2003-12-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2003/v20n4/OJOOBS_2003_v20n4_261.pdf
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spelling 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
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