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On some new aspects of the photo-gravitational Copenhagen problem

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dc.contributor.author Kalvouridis, TJ en
dc.date.accessioned 2014-03-01T01:28:55Z
dc.date.available 2014-03-01T01:28:55Z
dc.date.issued 2008 en
dc.identifier.issn 0004-640X en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/19031
dc.subject Celestial mechanics en
dc.subject Photo-gravitational Copenhagen problem en
dc.subject Stationary solutions en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.other RESTRICTED 3-BODY PROBLEM en
dc.subject.other 3 BODY PROBLEM en
dc.subject.other RADIATION PRESSURE en
dc.subject.other PERIODIC-ORBITS en
dc.subject.other EQUILIBRIUM POINTS en
dc.subject.other ASYMPTOTIC ORBITS en
dc.subject.other LIBRATION POINTS en
dc.subject.other STABILITY en
dc.subject.other FAMILIES en
dc.title On some new aspects of the photo-gravitational Copenhagen problem en
heal.type journalArticle en
heal.identifier.primary 10.1007/s10509-008-9861-0 en
heal.identifier.secondary http://dx.doi.org/10.1007/s10509-008-9861-0 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract We deal with some new aspects of the photo-gravitational Copenhagen case of the restricted three-body problem; more particularly, the distribution and the attracting domains of the stationary solutions of small particles that move in the neighborhood of two major bodies with equal masses when one or both primaries are radiation sources with constant luminosity. Under these conditions, each particle is subjected not only to gravitational forces but to the radiation emitted from the primaries as well. © 2008 Springer Science+Business Media B.V. en
heal.publisher SPRINGER en
heal.journalName Astrophysics and Space Science en
dc.identifier.doi 10.1007/s10509-008-9861-0 en
dc.identifier.isi ISI:000259935000016 en
dc.identifier.volume 317 en
dc.identifier.issue 1-2 en
dc.identifier.spage 107 en
dc.identifier.epage 117 en


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