Deformation of the gravitational field in ring-type N-body systems due to the presence of many radiation sources

Kazazakis, D; Kalvouridis, TJ

dc.contributor.author	Kazazakis, D	en
dc.contributor.author	Kalvouridis, TJ	en
dc.date.accessioned	2014-03-01T01:18:49Z
dc.date.available	2014-03-01T01:18:49Z
dc.date.issued	2003	en
dc.identifier.issn	0167-9295	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/15216
dc.subject	Equilibrium positions	en
dc.subject	N-body ring-type configurations	en
dc.subject	Radiation pressure	en
dc.subject	Zero-velocity curves	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Geosciences, Multidisciplinary	en
dc.subject.other	gravity	en
dc.subject.other	radiation exposure	en
dc.subject.other	theoretical study	en
dc.title	Deformation of the gravitational field in ring-type N-body systems due to the presence of many radiation sources	en
heal.type	journalArticle	en
heal.identifier.primary	10.1023/B:MOON.0000034495.99039.6f	en
heal.identifier.secondary	http://dx.doi.org/10.1023/B:MOON.0000034495.99039.6f	en
heal.language	English	en
heal.publicationDate	2003	en
heal.abstract	We study the distortion of the gravitational force field of an N-body ring-type cluster due to the presence of many radiation sources. We basically apply the Radzievskii's theory in this general model, considering that each member of the cluster is an independent radiation source. © 2004 Kluwer Academic Publishers.	en
heal.publisher	KLUWER ACADEMIC PUBL	en
heal.journalName	Earth, Moon and Planets	en
dc.identifier.doi	10.1023/B:MOON.0000034495.99039.6f	en
dc.identifier.isi	ISI:000222604200001	en
dc.identifier.volume	93	en
dc.identifier.issue	2	en
dc.identifier.spage	75	en
dc.identifier.epage	95	en