Dynamical stability of triple stars (Orlov+, 2000)

Details Dynamical stability of triple stars (Orlov+, 2000) Dynamical stability of triple stars (Orlov+, 2000)

Oct 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000ycat..90260301o&link_type=abstract

VizieR On-line Data Catalog: J/PAZh/26/301. Originally published in: 2000PAZh...26..301O; 2000AstL...26..250O

Computer Science

Stars: Double And Multiple, Binaries: Orbits, Stars: Masses

Scientific paper

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. (2 data files).

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