Areas of equatorial motion in the magnetic-binary problem

Kalvoridis, T; Mavraganis, A; Pangalos, C; Zagouras, Ch

dc.contributor.author	Kalvoridis, T	en
dc.contributor.author	Mavraganis, A	en
dc.contributor.author	Pangalos, C	en
dc.contributor.author	Zagouras, Ch	en
dc.date.accessioned	2014-03-01T01:06:23Z
dc.date.available	2014-03-01T01:06:23Z
dc.date.issued	1985	en
dc.identifier.issn	0008-8714	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/9351
dc.subject	Equilibrium Point	en
dc.subject	Steepest Descent Method	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Mechanics	en
dc.title	Areas of equatorial motion in the magnetic-binary problem	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF01230925	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF01230925	en
heal.language	English	en
heal.publicationDate	1985	en
heal.abstract	In the process of modelling the Magnetic-Binary systems, we deal with the permissible areas of motion in the equatorial planes of the representative model. The zero velocity curves, derived by the well known steepest descent method, provide the means for determining these areas. Further these curves reveal all the equilibrium points located on the above planes. © 1985 D. Reidel Publishing Company.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Celestial Mechanics	en
dc.identifier.doi	10.1007/BF01230925	en
dc.identifier.isi	ISI:A1985A977200005	en
dc.identifier.volume	37	en
dc.identifier.issue	2	en
dc.identifier.spage	161	en
dc.identifier.epage	170	en