Volume 619, November 2018
|Number of page(s)||16|
|Section||Catalogs and data|
|Published online||12 November 2018|
Multiplicity among solar-type stars
Université de Strasbourg, CNRS, Observatoire Astronomique de Strasbourg, MR 7550, 11, rue de l’Université, U, 67 000 Strasbourg, France
2 Observatoire Astronomique de l’Université de Genève, 51, chemin des Maillettes, 1290 Sauverny, Switzerland
Accepted: 2 August 2018
Context. The statistical properties of binary stars are clues for understanding their formation process. A radial velocity survey was carried on amongst nearby G-type stars and the results were published in 1991.
Aims. The survey of radial velocity measurements was extended towards K-type stars.
Methods. A sample of 261 K-type stars was observed with the spectrovelocimeter CORAVEL (COrrelation RAdial VELocities). Those stars with a variable radial velocity were detected on the basis of the P(Χ2) test. The orbital elements of the spectroscopic binaries were then derived.
Results. The statistical properties of binary stars were derived from these observations and published in 2003. We present the catalogue of the radial velocity measurements obtained with CORAVEL for all the K stars of the survey and the orbital elements derived for 34 spectroscopic systems. In addition, the catalogue contains eight G-type spectroscopic binaries that have received additional measurements since 1991 and for which the orbital elements are revised or derived for the first time.
Key words: solar neighborhood / binaries: spectroscopic / stars: solar-type / stars: late-type
Tables A.1 and A.2 are also available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/619/A81
© ESO 2018
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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