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High precision radial-velocity measurements of late-type evolved stars
Published online by Cambridge University Press: 12 April 2016
Abstract
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
- Information
- International Astronomical Union Colloquium , Volume 170: Precise Stellar Radial Velocities , 1999 , pp. 204 - 210
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
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