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

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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


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