| dc.contributor.author | Koen, Chris | |
| dc.date.accessioned | 2015-12-11T09:04:14Z | |
| dc.date.available | 2015-12-11T09:04:14Z | |
| dc.date.issued | 2014 | |
| dc.identifier.citation | Koen, 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.issn | 0035-8711 | |
| dc.identifier.uri | http://hdl.handle.net/10566/2017 | |
| dc.description.abstract | 1SWASP 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.language.iso | en | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.rights | Oxford Open. Articles published under the Oxford Open model are made freely available online immediately upon publication, without subscription barriers to access. | |
| dc.source.uri | http://dx.doi.org/doi:10.1093/mnras/stu751 | |
| dc.subject | Astronomy | en_US |
| dc.subject | Mathematics | en_US |
| dc.subject | South African Astronomical Observatory (SAAO) | en_US |
| dc.subject | Photometry | en_US |
| dc.subject | Hierarchical multiple star systems | |
| dc.title | Multicolour time series photometry of the variable star 1SWASP J234401.81−212229.1 | en_US |
| dc.type | Article | en_US |
| dc.privacy.showsubmitter | false | |
| dc.status.ispeerreviewed | true | |
| dc.description.accreditation | Web of Science | en_US |
