Spectroscopic Orbits of Xi-Piscium 60-Andromedae and XI-1-CETI

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

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 photoelectrically at Cambridge are combined to determine their orbits. A brief discussion of radial-velocity zero-point difficulties is presented.

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