Synthetic light curve models

dc.contributor.author	Banks, Timothy Stuart
dc.date.accessioned	2011-08-25T21:15:28Z
dc.date.accessioned	2022-10-30T18:45:10Z
dc.date.available	2011-08-25T21:15:28Z
dc.date.available	2022-10-30T18:45:10Z
dc.date.copyright	1989
dc.date.issued	1989
dc.identifier.uri	https://ir.wgtn.ac.nz/handle/123456789/25901
dc.description.abstract	The Synthetic Light Curve Packages of Budding, and Wilson & Devinney are used to obtain physical parameters of eclipsing binaries ,and photospheric disturbances where appropriate. The systems modeled are CG-Cygni, R Arae, XY Ursae Majoris, AE Phoenicis, RT Andromedae, AB Doradus, YY Eridani, and RT Sculptoris. The structure and strategy of Budding's Eclipsing Binary Light Curve Fitting program is considered in detail. An operating manual is provided for the Budding programs, which are found to deduce parameters in reasonable agreement with Hill's Light, the Wilson-Devinney programs, and Wood's Wink.	en_NZ
dc.format	pdf	en_NZ
dc.language	en_NZ
dc.language.iso	en_NZ
dc.publisher	Te Herenga Waka—Victoria University of Wellington	en_NZ
dc.title	Synthetic light curve models	en_NZ
dc.type	Text	en_NZ
vuwschema.type.vuw	Awarded Research Masters Thesis	en_NZ
thesis.degree.discipline	Physics	en_NZ
thesis.degree.grantor	Te Herenga Waka—Victoria University of Wellington	en_NZ
thesis.degree.level	Masters	en_NZ
thesis.degree.name	Master of Science	en_NZ

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