The equilibrium state in the Magnetic-Binary problem when the more massive primary is an oblate spheroid

Mavraganis, AG

dc.contributor.author	Mavraganis, AG	en
dc.date.accessioned	2014-03-01T01:06:00Z
dc.date.available	2014-03-01T01:06:00Z
dc.date.issued	1981	en
dc.identifier.issn	00088714	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/9109
dc.subject	Characteristic Polynomial	en
dc.subject	Equilibrium Point	en
dc.subject	Equilibrium State	en
dc.subject	Stationary State	en
dc.title	The equilibrium state in the Magnetic-Binary problem when the more massive primary is an oblate spheroid	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF01230732	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF01230732	en
heal.publicationDate	1981	en
heal.abstract	The author's aim is to study in this paper the stationary state of the planar Magnetic-Binary problem by taking into consideration the oblateness of the more massive primary, and then to investigate the stability of motion about the equilibrium points by means of the characteristic polynomial of the linearised variational equations. © 1981 D. Reidel Publishing Co.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Celestial Mechanics	en
dc.identifier.doi	10.1007/BF01230732	en
dc.identifier.volume	23	en
dc.identifier.issue	3	en
dc.identifier.spage	287	en
dc.identifier.epage	293	en