Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis

The UBV light curves of a close eclipsing binary SW Lyn were obtained with the observations made at the Sobaeksan Astronomy Observatory during 7 nights from September 1983 to March 1987. These light curves show asymmetry to the secondary minimum light and the asymmetry is larger at the shorter wavel...

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Main Authors: Ho-Il Kim, Wonyong Han, Woo-Baik Lee, Chun-Hwey Kim
Format: Article
Language:English
Published: The Korean Space Science Society 1995-12-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1995/v12n2/OJOOBS_1995_v12n2_196.pdf
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author Ho-Il Kim
Wonyong Han
Woo-Baik Lee
Chun-Hwey Kim
author_facet Ho-Il Kim
Wonyong Han
Woo-Baik Lee
Chun-Hwey Kim
author_sort Ho-Il Kim
collection DOAJ
description The UBV light curves of a close eclipsing binary SW Lyn were obtained with the observations made at the Sobaeksan Astronomy Observatory during 7 nights from September 1983 to March 1987. These light curves show asymmetry to the secondary minimum light and the asymmetry is larger at the shorter wavelength light curve. Assuming that the star spot makes the asymmetry, we employed the WD code to make the B and V light curves solution. We confirmed that SW Lyn has near contact (semi-detached) Roche configuration and has the Case A evolution.
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spelling doaj.art-5df4dd77c3624701bace488ed399e5242024-01-02T02:39:23ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14091995-12-01122196203Light Curve Analysis of a Short Period Eclipsing Binary SW LyncisHo-Il Kim0Wonyong Han1Woo-Baik Lee2Chun-Hwey Kim3Korea Astronomy Observatory, Taejon 305-348, KoreaKorea Astronomy Observatory, Taejon 305-348, KoreaKorea Astronomy Observatory, Taejon 305-348, KoreaDepartment of Astronomy and Space Science, Chungbuk National UniversityThe UBV light curves of a close eclipsing binary SW Lyn were obtained with the observations made at the Sobaeksan Astronomy Observatory during 7 nights from September 1983 to March 1987. These light curves show asymmetry to the secondary minimum light and the asymmetry is larger at the shorter wavelength light curve. Assuming that the star spot makes the asymmetry, we employed the WD code to make the B and V light curves solution. We confirmed that SW Lyn has near contact (semi-detached) Roche configuration and has the Case A evolution.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1995/v12n2/OJOOBS_1995_v12n2_196.pdf
spellingShingle Ho-Il Kim
Wonyong Han
Woo-Baik Lee
Chun-Hwey Kim
Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis
Journal of Astronomy and Space Sciences
title Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis
title_full Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis
title_fullStr Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis
title_full_unstemmed Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis
title_short Light Curve Analysis of a Short Period Eclipsing Binary SW Lyncis
title_sort light curve analysis of a short period eclipsing binary sw lyncis
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1995/v12n2/OJOOBS_1995_v12n2_196.pdf
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AT chunhweykim lightcurveanalysisofashortperiodeclipsingbinaryswlyncis