On the stability of the hypothetical quintet system of TW Draconis

dc.contributor.author	Abhyankar, K. D
dc.contributor.author	Bhatia, R. K
dc.contributor.author	Devadas Rao, P
dc.date.accessioned	2005-12-08T04:07:09Z
dc.date.available	2005-12-08T04:07:09Z
dc.date.issued	1985-09
dc.identifier.citation	BASI, Vol. 13, No. 3, pp. 275-286	en
dc.identifier.uri	http://hdl.handle.net/2248/662
dc.description.abstract	Aarseth`s NBODY 1 code is used to study the stability of the quintet system of DW Draconis postulated by Abhyankar & Panchatsaram (1984). It is found that the observed (O - C) curve based on the ephemeris by Tremko & Kreiner (1981) can be reproduced by taking appropriate initial conditions; but the system becomes unstable outside the range of observations. The nature of instability is studied.	en
dc.format.extent	687353 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Eclipsing binaries	en
dc.subject	Multiple system	en
dc.subject	n-body intergration	en
dc.title	On the stability of the hypothetical quintet system of TW Draconis	en
dc.type	Article	en