Photometric Study on the Spot-Double Star XY Ursae Majoris (II)

The photometric behaviour of XY UMa, an eclipsing binary showing photospheric and chromospheric activity, has been described by spot hypothesis. They are based on the all the available UBV light curves, which were carried out by Geyer since 1955. A "spherical rectangular" spot model shows...

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Main Author: Woo-Baik Lee
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 1988-12-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_97.pdf
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spelling doaj-77f6b4b5cbb24f1a806b343ffcadbc7d2020-11-25T01:56:37ZengKorean Space Science Society (KSSS)Journal of Astronomy and Space Sciences2093-55872093-14091988-12-015297109 Photometric Study on the Spot-Double Star XY Ursae Majoris (II)Woo-Baik Lee0Institute of Space Science and Astronomy, Daejeon 302-348The photometric behaviour of XY UMa, an eclipsing binary showing photospheric and chromospheric activity, has been described by spot hypothesis. They are based on the all the available UBV light curves, which were carried out by Geyer since 1955. A "spherical rectangular" spot model shows very pronounced spot activities during the last 30 years. On the average, the spot covered about 16% of the visible hemisphere. Observational evidence for photospheric and chromospheric activities on the XY UMa and related systems are also discussed.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_97.pdf
collection DOAJ
language English
format Article
sources DOAJ
author Woo-Baik Lee
spellingShingle Woo-Baik Lee
Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
Journal of Astronomy and Space Sciences
author_facet Woo-Baik Lee
author_sort Woo-Baik Lee
title Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
title_short Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
title_full Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
title_fullStr Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
title_full_unstemmed Photometric Study on the Spot-Double Star XY Ursae Majoris (II)
title_sort photometric study on the spot-double star xy ursae majoris (ii)
publisher Korean Space Science Society (KSSS)
series Journal of Astronomy and Space Sciences
issn 2093-5587
2093-1409
publishDate 1988-12-01
description The photometric behaviour of XY UMa, an eclipsing binary showing photospheric and chromospheric activity, has been described by spot hypothesis. They are based on the all the available UBV light curves, which were carried out by Geyer since 1955. A "spherical rectangular" spot model shows very pronounced spot activities during the last 30 years. On the average, the spot covered about 16% of the visible hemisphere. Observational evidence for photospheric and chromospheric activities on the XY UMa and related systems are also discussed.
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_97.pdf
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