Abstract
In this article we treat analytically the problem of finding stability limits ofP-type orbits (=direct nearly circular orbits surrounding both primaries) in double stars. The model used is the circular restricted three body problem; in that sense the results are not valid for binaries in eccentric orbits. But as the chosen model is often used in dynamical descriptions of the problem we can compare our results with other ones derived in earlier studies with semianalytical or just numerical methods.
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