Abstract
The orbital period variations of the eclipsing binary BX And are examined analysing its (O-C) diagram 1) with the standard method, in which the minima times are fitted by the quadratic ephemeris combined with an assumed light-time effect, and 2) with the first continuous method. The results from the use of the two methods are, as was expected, different.
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Rovithis-Livaniou, H., Tsantilas, S., Rovithis, P., Chochol, D., Skopal, A., Pribulla, T. (2005). The Eclipsing Binary BX Andromedae and its Orbital Period Behaviour. In: Drechsel, H., Zejda, M. (eds) Zdeněk Kopal’s Binary Star Legacy. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3875-5_9
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DOI: https://doi.org/10.1007/1-4020-3875-5_9
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