Attracting domains in ring-type N-body formations

Croustalloudi, M; Kalvouridis, T

dc.contributor.author	Croustalloudi, M	en
dc.contributor.author	Kalvouridis, T	en
dc.date.accessioned	2014-03-01T01:25:58Z
dc.date.available	2014-03-01T01:25:58Z
dc.date.issued	2007	en
dc.identifier.issn	0032-0633	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/17847
dc.subject	Attracting domains	en
dc.subject	Equilibrium states	en
dc.subject	N-body ring-type systems	en
dc.subject	Parametric variation of the equilibrium zones	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.other	Fractals	en
dc.subject.other	Gravitation	en
dc.subject.other	Iterative methods	en
dc.subject.other	Attracting domains	en
dc.subject.other	Equilibrium zones	en
dc.subject.other	Space research	en
dc.title	Attracting domains in ring-type N-body formations	en
heal.type	journalArticle	en
heal.identifier.primary	10.1016/j.pss.2006.04.008	en
heal.identifier.secondary	http://dx.doi.org/10.1016/j.pss.2006.04.008	en
heal.language	English	en
heal.publicationDate	2007	en
heal.abstract	The objective of our paper is the investigation of the attracting domains, namely the sets consisting of the initial points for which the application of an iterative process leads to the equilibrium positions of a small body, upon which act the gravitational forces of N big bodies arranged in a ring-type configuration. We describe the process to form these areas and we investigate their dependence on the two parameters of the system. The results obtained, in many cases show a fractal-type structure of these regions. (c) 2006 Elsevier Ltd. All rights reserved.	en
heal.publisher	PERGAMON-ELSEVIER SCIENCE LTD	en
heal.journalName	Planetary and Space Science	en
dc.identifier.doi	10.1016/j.pss.2006.04.008	en
dc.identifier.isi	ISI:000243803500005	en
dc.identifier.volume	55	en
dc.identifier.issue	1-2	en
dc.identifier.spage	53	en
dc.identifier.epage	69	en