Multicolour time series photometry of the variable star 1SWASP J234401.81−212229.1

dc.contributor.authorKoen, Chris
dc.date.accessioned2015-12-11T09:04:14Z
dc.date.available2015-12-11T09:04:14Z
dc.date.issued2014
dc.description.abstract1SWASP J234401.81-212229.1 may be one of a handful of contact binaries comprising two Mdwarfs. Modelling of the available observations is complicated by the fact that the radiation of the eclipsing system is dominated by a third star, a K dwarf. New photometry, presented in this paper, strengthens this interpretation of the data. The existence of such systems will have implications for the statistical distributions of masses in hierarchical multiple star systems.en_US
dc.description.accreditationWeb of Scienceen_US
dc.identifier.citationKoen, C. (2014). Multicolour time series photometry of the variable star 1SWASP J234401.81−212229.1. Monthly Notices of the Royal Astronomical Society, 441 (4): 3075-3082.en_US
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/10566/2017
dc.language.isoenen_US
dc.privacy.showsubmitterfalse
dc.publisherOxford University Pressen_US
dc.rightsOxford Open. Articles published under the Oxford Open model are made freely available online immediately upon publication, without subscription barriers to access.
dc.source.urihttp://dx.doi.org/doi:10.1093/mnras/stu751
dc.status.ispeerreviewedtrue
dc.subjectAstronomyen_US
dc.subjectMathematicsen_US
dc.subjectSouth African Astronomical Observatory (SAAO)en_US
dc.subjectPhotometryen_US
dc.subjectHierarchical multiple star systems
dc.titleMulticolour time series photometry of the variable star 1SWASP J234401.81−212229.1en_US
dc.typeArticleen_US

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