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On the period variations of RT Persei
Authors:S Mancuso  L Milano
Institution:1. Capodimonte Astronomical Observatory, Naples, Italy
Abstract:The observed minima of RT Persei up to 1971 are collected and treated by the method of least squares to establish periodic terms with a fundamental period of 40y0 and, furthermore, a quadratic term. It is shown that the periodic terms might be explained by the presence of a third body, but this hypothesis seems unlikely, and could be definitively ruled out by new spectroscopic observations. A dynamical instability of the system may constitute a more likely explanation of the observed period changes.
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