Stability VS inclination of motions in E3

Halioulias, A; Katsiaris, GA; Markellos, VV

dc.contributor.author	Halioulias, A	en
dc.contributor.author	Katsiaris, GA	en
dc.contributor.author	Markellos, VV	en
dc.date.accessioned	2014-03-01T01:37:49Z
dc.date.available	2014-03-01T01:37:49Z
dc.date.issued	1976	en
dc.identifier.issn	0004640X	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/21762
dc.title	Stability VS inclination of motions in E3	en
heal.type	journalArticle	en
heal.identifier.primary	10.1007/BF00646190	en
heal.identifier.secondary	http://dx.doi.org/10.1007/BF00646190	en
heal.publicationDate	1976	en
heal.abstract	Five families of three-dimensional doubly symmetric motions are computed after establishing their existence by means of a grid-search technique. It is confirmed that within the same family orbits of lower inclination with respect to the plane of motion of the primaries are stable while the critical inclination at which instability occurs varies between families. The maximum inclination at which stable motions of the type presented here were found is about 52°. © 1976 D. Reidel Publishing Company.	en
heal.publisher	Kluwer Academic Publishers	en
heal.journalName	Astrophysics and Space Science	en
dc.identifier.doi	10.1007/BF00646190	en
dc.identifier.volume	41	en
dc.identifier.issue	2	en
dc.identifier.spage	417	en
dc.identifier.epage	422	en