WASP light curve of the eclipsing binary VZ CVn

WASP light curve of the eclipsing binary VZ CVn

The WASP light curve of the eclipsing binary VZ CVn, consisting of more than 14000 individual observations, is analyzed for photometric elements using the modeling code of Đurašević (1992). The spectroscopic parameters are adopted from the recent radial velocity work by Pribulla et al. (200...

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Main Author: Latković O.
Format: Article
Language:English
Published: Astronomical Observatory, Department of Astronomy, Belgrade 2012-01-01
Series:Serbian Astronomical Journal
Subjects:
binaries: eclipsing
binaries: spectroscopic
stars: individual: VZ CVn
Online Access:http://www.doiserbia.nb.rs/img/doi/1450-698X/2012/1450-698X1284077L.pdf
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spelling doaj-96cf486fa1704a698623a85e682c4f532020-11-24T21:38:03ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X1820-92892012-01-012012184778210.2298/SAJ1284077L1450-698X1284077LWASP light curve of the eclipsing binary VZ CVnLatković O.0Astronomical Observatory, BelgradeThe WASP light curve of the eclipsing binary VZ CVn, consisting of more than 14000 individual observations, is analyzed for photometric elements using the modeling code of Đurašević (1992). The spectroscopic parameters are adopted from the recent radial velocity work by Pribulla et al. (2009). The results of the study include new times of minimum light, an improved ephemeris, and the updated physical and orbital parameters of the system.http://www.doiserbia.nb.rs/img/doi/1450-698X/2012/1450-698X1284077L.pdfbinaries: eclipsingbinaries: spectroscopicstars: individual: VZ CVn
collection DOAJ
language English
format Article
sources DOAJ
author Latković O.
spellingShingle Latković O.
WASP light curve of the eclipsing binary VZ CVn
Serbian Astronomical Journal
binaries: eclipsing
binaries: spectroscopic
stars: individual: VZ CVn
author_facet Latković O.
author_sort Latković O.
title WASP light curve of the eclipsing binary VZ CVn
title_short WASP light curve of the eclipsing binary VZ CVn
title_full WASP light curve of the eclipsing binary VZ CVn
title_fullStr WASP light curve of the eclipsing binary VZ CVn
title_full_unstemmed WASP light curve of the eclipsing binary VZ CVn
title_sort wasp light curve of the eclipsing binary vz cvn
publisher Astronomical Observatory, Department of Astronomy, Belgrade
series Serbian Astronomical Journal
issn 1450-698X
1820-9289
publishDate 2012-01-01
description The WASP light curve of the eclipsing binary VZ CVn, consisting of more than 14000 individual observations, is analyzed for photometric elements using the modeling code of Đurašević (1992). The spectroscopic parameters are adopted from the recent radial velocity work by Pribulla et al. (2009). The results of the study include new times of minimum light, an improved ephemeris, and the updated physical and orbital parameters of the system.
topic binaries: eclipsing
binaries: spectroscopic
stars: individual: VZ CVn
url http://www.doiserbia.nb.rs/img/doi/1450-698X/2012/1450-698X1284077L.pdf
work_keys_str_mv AT latkovico wasplightcurveoftheeclipsingbinaryvzcvn
_version_ 1725935751791640576

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