dc.contributor.author |
Kalvouridis, TJ |
en |
dc.contributor.author |
Mavraganis, AG |
en |
dc.date.accessioned |
2014-03-01T01:10:57Z |
|
dc.date.available |
2014-03-01T01:10:57Z |
|
dc.date.issued |
1995 |
en |
dc.identifier.issn |
0004-640X |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/11519 |
|
dc.subject |
Stationary Solution |
en |
dc.subject.classification |
Astronomy & Astrophysics |
en |
dc.subject.other |
LIBRATION POINTS |
en |
dc.subject.other |
3-BODY PROBLEM |
en |
dc.subject.other |
RADIATION PRESSURE |
en |
dc.subject.other |
3 BODIES |
en |
dc.title |
Equilibria and stability of the restricted photogravitational problem of 2 + 2 bodies |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1007/BF00626906 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1007/BF00626906 |
en |
heal.language |
English |
en |
heal.publicationDate |
1995 |
en |
heal.abstract |
The restricted problem of 2 + 2 bodies when one of the infinitesimal masses is further acted upon by the light pressure of the two primaries, is considered. The stationary solutions of this problem are found out. A short discussion is devoted to the stability of these solutions. © 1995 Kluwer Academic Publishers. |
en |
heal.publisher |
Kluwer Academic Publishers |
en |
heal.journalName |
Astrophysics and Space Science |
en |
dc.identifier.doi |
10.1007/BF00626906 |
en |
dc.identifier.isi |
ISI:A1995RH58300014 |
en |
dc.identifier.volume |
226 |
en |
dc.identifier.issue |
1 |
en |
dc.identifier.spage |
137 |
en |
dc.identifier.epage |
148 |
en |