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High precision radial-velocity measurements of late-type evolved stars

Published online by Cambridge University Press:  12 April 2016

I.N. Cummings
Affiliation:
Mt John University Observatory, Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand
J.B. Hearnshaw
Affiliation:
Mt John University Observatory, Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand
P.M. Kilmartin
Affiliation:
Mt John University Observatory, Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand
A.C. Gilmore
Affiliation:
Mt John University Observatory, Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand

Abstract

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High dispersion spectra for 44 southern evolved stars of spectral type K or M have been obtained. From these observations relative radial velocities of 50 m/s precision have been obtained by the method of digital cross-correlation. This method of achieving precise relative radial velocities for late-type stars, and the problems encountered in its use, are discussed. Using this method, statistically significant radial-velocity variations have been found. Two of the observed stars have their precise radial velocities presented and the potential mechanisms of their variation examined.

Type
Part 5. Variable Stars
Copyright
Copyright © Astronomical Society of the Pacific 1999

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