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• W4206561293 abstract "The Wilson–Devinney model has—over the last 50 years—become the standard in analyzing eclipsing binary observations. To provide orientation for both active binary and non-binary researchers, it is presented here in historical and on-going as well as astrophysical perspectives. Among the important advances that originated with the model are: the representation of star surfaces as equipotentials for circular and eccentric orbits, leading to four morphological types; simultaneous least-squares light and velocity curve analyses; efficient reflection computation, including multiple reflection; disk theory and disk modeling. Solutions in physical units allowed for the accurate estimation of parameters such as stellar masses and photometric distances; inclusion of types of observables, properly weighted." @default.
• W4206561293 created "2022-01-25" @default.
• W4206561293 creator A5081209307 @default.
• W4206561293 date "2022-01-19" @default.
• W4206561293 modified "2023-09-30" @default.
• W4206561293 title "Fifty Years of Eclipsing Binary Analysis with the Wilson–Devinney Model" @default.
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• W4206561293 doi "https://doi.org/10.3390/galaxies10010017" @default.
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