Modelling of eclipsing binaries
W Ursae Majoris-type (W UMa-type) variable stars are contact eclipsing binary stars whose evolution is unknown. Modelling to determine the physical parameters of as many W UMa-type variable stars as possible might provide some insight as to how these contact binaries form and evolve. The All Sky...
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| Format: | Others |
| Language: | en |
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2010
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| Online Access: | http://hdl.handle.net/10500/3099 |