Cover: Planetary motion in binary star systems, preliminary results

Planetary motion in binary star systems, preliminary results

Published 1978

by Stephen H. Dole

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Computer simulations of planetary motion in binary star systems were carried out to determine the maximum extent of the circumstellar region in which stable near-circular orbits can exist as a function of stellar mass ratio and orbital eccentricity. Preliminary results for direct, in-plane, planetary motion are presented.

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