Light curve analysis of the late type binary V523 Cassiopeiae
We present the analysis of V and R light curves of the late type contact binary V523 Cas for the season of 2006. These observations make part of the monitoring program aimed at studying the long-term light curve variability in this system. Our results confirm that the system is in an over contact co...
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Astronomical Observatory, Department of Astronomy, Belgrade
2009-01-01
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doaj-035f509fdf964590984196abb75c1ab22020-11-24T22:47:42ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892009-01-012009178454810.2298/SAJ0978045L1450-698X0978045LLight curve analysis of the late type binary V523 CassiopeiaeLatković O.0Zboril M.1Đurašević G.2Astronomical Observatory, BelgradeAstronomical Institute, Tatranská Lomnica, SlovakiaAstronomical Observatory, BelgradeWe present the analysis of V and R light curves of the late type contact binary V523 Cas for the season of 2006. These observations make part of the monitoring program aimed at studying the long-term light curve variability in this system. Our results confirm that the system is in an over contact configuration, and include a bright spot in the neck region of the cooler and larger primary. We compare these results with the previous solution, obtained for the season 2005 dataset and discuss the differences.http://www.doiserbia.nb.rs/img/doi/1450-698X/2009/1450-698X0978045L.pdfbinaries, closebinaries, eclipsingstars, individual, V523 Casstars, late-typestars, activity |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Latković O. Zboril M. Đurašević G. |
spellingShingle |
Latković O. Zboril M. Đurašević G. Light curve analysis of the late type binary V523 Cassiopeiae Serbian Astronomical Journal binaries, close binaries, eclipsing stars, individual, V523 Cas stars, late-type stars, activity |
author_facet |
Latković O. Zboril M. Đurašević G. |
author_sort |
Latković O. |
title |
Light curve analysis of the late type binary V523 Cassiopeiae |
title_short |
Light curve analysis of the late type binary V523 Cassiopeiae |
title_full |
Light curve analysis of the late type binary V523 Cassiopeiae |
title_fullStr |
Light curve analysis of the late type binary V523 Cassiopeiae |
title_full_unstemmed |
Light curve analysis of the late type binary V523 Cassiopeiae |
title_sort |
light curve analysis of the late type binary v523 cassiopeiae |
publisher |
Astronomical Observatory, Department of Astronomy, Belgrade |
series |
Serbian Astronomical Journal |
issn |
1450-698X 1820-9289 |
publishDate |
2009-01-01 |
description |
We present the analysis of V and R light curves of the late type contact binary V523 Cas for the season of 2006. These observations make part of the monitoring program aimed at studying the long-term light curve variability in this system. Our results confirm that the system is in an over contact configuration, and include a bright spot in the neck region of the cooler and larger primary. We compare these results with the previous solution, obtained for the season 2005 dataset and discuss the differences. |
topic |
binaries, close binaries, eclipsing stars, individual, V523 Cas stars, late-type stars, activity |
url |
http://www.doiserbia.nb.rs/img/doi/1450-698X/2009/1450-698X0978045L.pdf |
work_keys_str_mv |
AT latkovico lightcurveanalysisofthelatetypebinaryv523cassiopeiae AT zborilm lightcurveanalysisofthelatetypebinaryv523cassiopeiae AT đurasevicg lightcurveanalysisofthelatetypebinaryv523cassiopeiae |
_version_ |
1725680872611381248 |