Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12
| Contribuinte(s) |
Universidade Estadual Paulista (UNESP) |
|---|---|
| Data(s) |
26/02/2014
20/05/2014
26/02/2014
20/05/2014
01/04/2006
|
| Resumo |
This paper considers the dynamics of two planets, as the planets B and C of the pulsar PSR B1257+12, near a 3/2 mean-motion resonance. A two-degrees-of-freedom model, in the framework of the general three-body planar problem, is used and the solutions are analyzed through surfaces of section and Fourier techniques in the full phase space of the system. |
| Formato |
381-397 |
| Identificador |
http://dx.doi.org/10.1007/s10569-006-9002-4 Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006. 0923-2958 http://hdl.handle.net/11449/24846 10.1007/s10569-006-9002-4 WOS:000238517200002 |
| Idioma(s) |
eng |
| Publicador |
Springer |
| Relação |
Celestial Mechanics & Dynamical Astronomy |
| Direitos |
closedAccess |
| Palavras-Chave | #chaos #extra-solar planets #planetary systems #pulsar planets #resonance |
| Tipo |
info:eu-repo/semantics/article |
