Symmetric motions in the Equatorial Magnetic-Binary Problem

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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

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