Zero-velocity surfaces in the three-dimensional ring problem of N+1 bodies

Kalvouridis, TJ

dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T01:17:20Z
dc.date.available	2014-03-01T01:17:20Z
dc.date.issued	2001	en
dc.identifier.issn	0923-2958	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/14462
dc.subject	zero-velocity surfaces	en
dc.subject	ring problem	en
dc.subject	N-body configurations	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Mathematics, Interdisciplinary Applications	en
dc.subject.other	RESTRICTED 4-BODY PROBLEMS	en
dc.title	Zero-velocity surfaces in the three-dimensional ring problem of N+1 bodies	en
heal.type	journalArticle	en
heal.identifier.primary	10.1023/A:1011919508410	en
heal.identifier.secondary	http://dx.doi.org/10.1023/A:1011919508410	en
heal.language	English	en
heal.publicationDate	2001	en
heal.abstract	The zero-velocity surfaces in the three-dimensional ring problem of N + 1 bodies and their parametric evolution is the subject of this paper. These surfaces, which are also known as Hill's or Jacobian surfaces, provide us with valuable information concerning the regions of the permissible particle motion and the existence of equilibrium positions.	en
heal.publisher	KLUWER ACADEMIC PUBL	en
heal.journalName	CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY	en
dc.identifier.doi	10.1023/A:1011919508410	en
dc.identifier.isi	ISI:000172046600005	en
dc.identifier.volume	80	en
dc.identifier.issue	2	en
dc.identifier.spage	133	en
dc.identifier.epage	144	en