On the stability of the hypothetical quintet system of TW Draconis

Details On the stability of the hypothetical quintet system of TW Draconis On the stability of the hypothetical quintet system of TW Draconis

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13..275a&link_type=abstract

Astronomical Society of India, Bulletin, vol. 13, Sept. 1985, p. 275-286.

Statistics

Computation

2

Computational Astrophysics, Eclipsing Binary Stars, Many Body Problem, Stellar Orbits, Numerical Integration, Systems Stability

Scientific paper

Aarseth's (1971) NBODY 1 code is used to study the stability of the quintet system of DW Draconis postulated by Abhyankar and Panchatsaram (1984). It is found that the observed (O-C) curve based on the ephemeris by Tremko and Kreiner (1981) can be reproduced by taking appropriate initial conditions, but that the system becomes unstable outside the range of observations. The nature of instability is studied.

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