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

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dc.contributor.author Kalvouridis, TJ en
dc.date.accessioned 2014-03-01T01:51:25Z
dc.date.available 2014-03-01T01:51:25Z
dc.date.issued 2001 en
dc.identifier.issn 0923-2958 en
dc.identifier.uri http://hdl.handle.net/123456789/26279
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.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.isi ISI:000171141000005 en
dc.identifier.volume 80 en
dc.identifier.issue 2 en
dc.identifier.spage 133 en
dc.identifier.epage 144 en


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