Dynamical stability of triple stars Virtual Observatory Resource

Authors
  1. Orlov V.V.
  2. Petrova A.V.
  3. Published by
    CDS
Abstract

The dynamic stability of 38 observed hierarchical triple stars with known orbital elements of the internal and external binary subsystems and component masses is considered. Four different criteria of dynamical stability are used. The observed stability parameters and their critical values are calculated by taking into account errors in the orbital elements and component masses.

Keywords
  1. Multiple stars
  2. Orbits
  3. Stellar masses
Bibliographic source Bibcode
2000PAZh...26..301O
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/26/301
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PAZh/26/301

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/PAZh/26/301
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/26/301
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/26/301
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2000-10-31T22:43:13Z
Resource record created
2000-10-31T21:44:21Z
Updated
2000-10-31T22:43:13Z
Created

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr