Orbits of {beta} Ret and {nu} Oct Virtual Observatory Resource

Authors

1. Ramm D.J.
2. Pourbaix D.
3. Hearnshaw J.B.
4. Komonjinda S.

Published by

CDS

Abstract

New astrometric-spectroscopic orbital solutions for the single-line K-giant binaries beta Reticuli (P~5.2yr, e=0.3346+/-0.0004) and nu Octantis (P~2.9yr, e=0.2358+/-0.0003) have been derived based on high-precision spectroscopic radial velocities (RVs) and the Hipparcos astrometry.

Keywords

1. spectroscopic-binary-stars
2. solar-system-planets
3. radial-velocity

Bibliographic source Bibcode

2009MNRAS.394.1695R

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/394/1695

IVOA Identifier IVOID

ivo://CDS.VizieR/J/MNRAS/394/1695

Document Object Identifer DOI

doi:10.26093/cds/vizier.73941695

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/394/1695
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/394/1695
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/394/1695

IVOA Table Access TAP

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