The triple system ADS 9167

It is found from the observations with the correlation radial velocity meter that the primary component of the visual double star ADS 9167 is a single-lined spectroscopic binary with 2.87- yr period and 0.75 eccentricity. Using the 26-year-long series of Pulkovo photographic relative-positions observations, a new visual orbit of AB is calculated with a period of about 1000 years.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/PAZh/24/868
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/24/868
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PAZh/24/868
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/PAZh/24/868
Provenance
Creator Kiyaeva O.V.; Tokovinin A.A.; Kalinichenko O.A.
Publisher CDS
Publication Year 1999
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Exoplanet Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy