Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis

A total of 546 UBV photoelectric observations of AG Per was carried out from January to December in 1993 at Chungbuk National University Observatory. With our observations, UBV light curves were constructed, three minimum times of JDHel. 2449284.213, JDHel. 2449360.060, and JDHel. 2449363.192 were d...

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Main Authors: K. H. Lee, J. H. Jeong
Format: Article
Language:English
Published: The Korean Space Science Society 1996-06-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1996/v13n1/OJOOBS_1996_v13n1_63.pdf
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author K. H. Lee
J. H. Jeong
author_facet K. H. Lee
J. H. Jeong
author_sort K. H. Lee
collection DOAJ
description A total of 546 UBV photoelectric observations of AG Per was carried out from January to December in 1993 at Chungbuk National University Observatory. With our observations, UBV light curves were constructed, three minimum times of JDHel. 2449284.213, JDHel. 2449360.060, and JDHel. 2449363.192 were determined. The phase displacement of secondary minimum time ¥ä=-0.046 were determined and orbital eccentricity e=0.071 was calculated. Forty-five times of minimum light (including ours) were collected from the literature and plotted on O-C diagram. We analyzed these data and apsidal motion period of U=76.17 (years) was obtained. Using e and U for AG Per, the internal structure constant, log k2, was found to be -2.13.
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spelling doaj.art-804452d028cb4e5ea1ef8f1d9e07f3912024-01-02T13:13:43ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14091996-06-011316371Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion AnalysisK. H. Lee0J. H. Jeong1Department of Astronomy and Space Science, Chungbuk National UniversityDepartment of Astronomy and Space Science, Chungbuk National UniversityA total of 546 UBV photoelectric observations of AG Per was carried out from January to December in 1993 at Chungbuk National University Observatory. With our observations, UBV light curves were constructed, three minimum times of JDHel. 2449284.213, JDHel. 2449360.060, and JDHel. 2449363.192 were determined. The phase displacement of secondary minimum time ¥ä=-0.046 were determined and orbital eccentricity e=0.071 was calculated. Forty-five times of minimum light (including ours) were collected from the literature and plotted on O-C diagram. We analyzed these data and apsidal motion period of U=76.17 (years) was obtained. Using e and U for AG Per, the internal structure constant, log k2, was found to be -2.13.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1996/v13n1/OJOOBS_1996_v13n1_63.pdf
spellingShingle K. H. Lee
J. H. Jeong
Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis
Journal of Astronomy and Space Sciences
title Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis
title_full Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis
title_fullStr Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis
title_full_unstemmed Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis
title_short Photoelectric Observations of Close Binary AG Persei and its Apsidal Motion Analysis
title_sort photoelectric observations of close binary ag persei and its apsidal motion analysis
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1996/v13n1/OJOOBS_1996_v13n1_63.pdf
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