BVRI Photometry of VV Cephei

UBV observations of VV Cep were made in 1988-1992 as a part of the Ten-year Observing Program for Long Period Eclipsing Binary Stars (1982-1992) at Yonsei University Observatory. In addition to these the observations in the longer passbands in R and I are also made in the 1991-1992 season at the sam...

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Main Authors: Il-Seong Nha, Hong-Seo Im, Yong-Sam Lee, Jang-Hae Jeong
Format: Article
Language:English
Published: The Korean Space Science Society 1992-06-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_89.pdf
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author Il-Seong Nha
Hong-Seo Im
Yong-Sam Lee
Jang-Hae Jeong
author_facet Il-Seong Nha
Hong-Seo Im
Yong-Sam Lee
Jang-Hae Jeong
author_sort Il-Seong Nha
collection DOAJ
description UBV observations of VV Cep were made in 1988-1992 as a part of the Ten-year Observing Program for Long Period Eclipsing Binary Stars (1982-1992) at Yonsei University Observatory. In addition to these the observations in the longer passbands in R and I are also made in the 1991-1992 season at the same observatory. Atmospheric extinction coefficient by a comparison star 20 Cep for B and V each night have been deduced a linear relation, kB = 0.159 + 1.066kV. In this paper, light curves of this star in BVRI passbands for the 1991-1992 season only are presented. Two periodic light variation of both long-term and short-term are found as for 90 days, respectively.
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spelling doaj.art-7a7f92feadf945fca88e8eb306ab71fc2024-02-02T12:13:04ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14091992-06-01918996BVRI Photometry of VV CepheiIl-Seong Nha0Hong-Seo Im1Yong-Sam Lee2Jang-Hae Jeong3Yonsei University Observatory, Seoul 120-749, KoreaYonsei University Observatory, Seoul 120-749, KoreaDepartment of Astronomy and Space Science, Chungbuk National University, Cheongju 361-763, KoreDepartment of Astronomy and Space Science, Chungbuk National University, Cheongju 361-763, KoreUBV observations of VV Cep were made in 1988-1992 as a part of the Ten-year Observing Program for Long Period Eclipsing Binary Stars (1982-1992) at Yonsei University Observatory. In addition to these the observations in the longer passbands in R and I are also made in the 1991-1992 season at the same observatory. Atmospheric extinction coefficient by a comparison star 20 Cep for B and V each night have been deduced a linear relation, kB = 0.159 + 1.066kV. In this paper, light curves of this star in BVRI passbands for the 1991-1992 season only are presented. Two periodic light variation of both long-term and short-term are found as for 90 days, respectively.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_89.pdf
spellingShingle Il-Seong Nha
Hong-Seo Im
Yong-Sam Lee
Jang-Hae Jeong
BVRI Photometry of VV Cephei
Journal of Astronomy and Space Sciences
title BVRI Photometry of VV Cephei
title_full BVRI Photometry of VV Cephei
title_fullStr BVRI Photometry of VV Cephei
title_full_unstemmed BVRI Photometry of VV Cephei
title_short BVRI Photometry of VV Cephei
title_sort bvri photometry of vv cephei
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1992/v9n1/OJOOBS_1992_v9n1_89.pdf
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AT yongsamlee bvriphotometryofvvcephei
AT janghaejeong bvriphotometryofvvcephei