The W Ursae Majoris systems : interpretation of light curves and line profiles
A method for the computer synthesis of theoretical light curves and like profiles for close binary stars in general has been developed and applied to the W Ursae Majoris stars. The geometry has been calculated using the centrally-condensed Roche model, for which a formulation in terms of cylindrical...
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| Language: | en |
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University of Canterbury. Chemistry
2013
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| Online Access: | http://hdl.handle.net/10092/8167 |