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Effective radii of Roche lobes were computed and are compared with the results of Kopal and of Pacynski. A convenient approximation is given, whose derivative is smooth and fairly accurate.
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P. P. Eggleton (Sun,) studied this question.
www.synapsesocial.com/papers/6a03c7bd3a92041adea9cc35 — DOI: https://doi.org/10.1086/160960
P. P. Eggleton
The Astrophysical Journal
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