Symmetric motions in the Equatorial Magnetic-Binary Problem

Kalvouridis, TJ; Mavraganis, AG

dc.contributor.author	Kalvouridis, TJ	en
dc.contributor.author	Mavraganis, AG	en
dc.date.accessioned	2014-03-01T01:07:00Z
dc.date.available	2014-03-01T01:07:00Z
dc.date.issued	1987	en
dc.identifier.issn	0008-8714	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/9727
dc.subject	Numerical Technique	en
dc.subject	Periodic Orbit	en
dc.subject	Variational Method	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Mechanics	en
dc.title	Symmetric motions in the Equatorial Magnetic-Binary Problem	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF01230259	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF01230259	en
heal.language	English	en
heal.publicationDate	1987	en
heal.abstract	Classical numerical techniques are applied to find families of symmetric periodic orbits in the Equatorial Magnetic-Binary Problem. Stability for each orbit is also studied by means of variational methods. Finally an example in a concrete system is given to verify the procedure proposed. © 1987 D. Reidel Publishing Company.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Celestial Mechanics	en
dc.identifier.doi	10.1007/BF01230259	en
dc.identifier.isi	ISI:A1987K734600006	en
dc.identifier.volume	40	en
dc.identifier.issue	2	en
dc.identifier.spage	177	en
dc.identifier.epage	196	en