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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/662
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dc.contributor.authorAbhyankar, K. D-
dc.contributor.authorBhatia, R. K-
dc.contributor.authorDevadas Rao, P-
dc.date.accessioned2005-12-08T04:07:09Z-
dc.date.available2005-12-08T04:07:09Z-
dc.date.issued1985-09-
dc.identifier.citationBASI, Vol. 13, No. 3, pp. 275-286en
dc.identifier.urihttp://hdl.handle.net/2248/662-
dc.description.abstractAarseth`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.extent687353 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectEclipsing binariesen
dc.subjectMultiple systemen
dc.subjectn-body intergrationen
dc.titleOn the stability of the hypothetical quintet system of TW Draconisen
dc.typeArticleen
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