Spectroscopic orbits of three K dwarf stars Virtual Observatory Resource

Authors

1. Tokovinin A.A.
2. Duquennoy A.
3. Halbwachs J.-L.
4. Mayor M.

Published by

CDS

Abstract

The spectroscopic orbits of single-lined binary dwarfs HD 23439B, HD 237287 and HD 217580 are derived from the radial velocities measured with two correlation radial-velocity spectrometers: correlation radial velocity (CORAVEL) at the 1m Swiss telescope of Observatoire de Haute-Provence, and radial velocity meters (RVM) used on several telescopes. The mutual agreement of these two data sets is analyzed and found to be quite good. The estimated minimum mass of secondary component corresponds to that of M-type dwarf for the first 2 systems and is equal to 0.06 solar mass for HD 217580.

Keywords

1. spectroscopic-binary-stars
2. radial-velocity
3. k-stars

Bibliographic source Bibcode

1994A&A...282..831T

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/282/831

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/282/831

Document Object Identifer DOI

doi:10.26093/cds/vizier.32820831

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/282/831
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/282/831
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/282/831

IVOA Table Access TAP

https://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).