Spectroscopic orbits of Piscium 60 Andromedae and 1 Ceti

Abstract
The three stars referred to in this paper are all fourth-magnitude late-type giants which have long been known to exhibit small variations in radial velocity. Velocities measured photographically at Lick and photo-electrically at Cambridge are combined to determine their orbits. A brief discussion of radial-velocity zero-point difficulties is presented.

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