Abstract
Based on spot model and Roche approximation for binary stars, the photometric analysis was carried out for the BV light curves of both the eclipsing system ER Vul and the non-eclipsing V711 Tau. The preferable spot parameters were obtained by using differential correction adjustment and least squares technique.
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© 1993 Springer-Verlag New York, Inc.
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Zhai, D.S., Zhang, R.X., Zhang, X.B. (1993). Spot Solutions for Two RS CVn Systems: ER Vul and V711 Tau. In: Milone, E.F. (eds) Light Curve Modeling of Eclipsing Binary Stars. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2742-7_16
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DOI: https://doi.org/10.1007/978-1-4612-2742-7_16
Publisher Name: Springer, New York, NY
Print ISBN: 978-1-4612-7649-4
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