Charged particles' areas of three-dimensional motions in a system of two magnetic stars

Kalvouridis, TJ

dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T01:29:58Z
dc.date.available	2014-03-01T01:29:58Z
dc.date.issued	2009	en
dc.identifier.issn	0004-640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/19427
dc.subject	Systems of magnetic binary stars	en
dc.subject	Zero-velocity surfaces	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.other	BINARY PROBLEM	en
dc.subject.other	SYMPLECTIC CHARACTER	en
dc.subject.other	EQUILIBRIUM POINTS	en
dc.subject.other	STABILITY	en
dc.subject.other	DIPOLES	en
dc.subject.other	FIELD	en
dc.title	Charged particles' areas of three-dimensional motions in a system of two magnetic stars	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/s10509-008-9970-9	en
heal.identifier.secondary	http://dx.doi.org/10.1007/s10509-008-9970-9	en
heal.language	English	en
heal.publicationDate	2009	en
heal.abstract	We study the parametric evolution of the regions where three-dimensional motions of a charged particle are allowed in the combined electromagnetic field produced by two rotating magnetic stars. We discuss the changes in the topology of the zero-velocity surfaces, as well as in the trapping regions of the particle motion for various values of the dipoles' magnetic moments. © 2008 Springer Science+Business Media B.V.	en
heal.publisher	SPRINGER	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1007/s10509-008-9970-9	en
dc.identifier.isi	ISI:000263159300003	en
dc.identifier.volume	319	en
dc.identifier.issue	2-4	en
dc.identifier.spage	105	en
dc.identifier.epage	114	en