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Please use this identifier to cite or link to this item: http://acervodigital.unesp.br/handle/11449/24846
Title: 
Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12
Author(s): 
Institution: 
  • Universidade Estadual Paulista (UNESP)
  • Universidade de São Paulo (USP)
ISSN: 
0923-2958
Abstract: 
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.
Issue Date: 
1-Apr-2006
Citation: 
Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006.
Time Duration: 
381-397
Publisher: 
Springer
Keywords: 
  • chaos
  • extra-solar planets
  • planetary systems
  • pulsar planets
  • resonance
Source: 
http://dx.doi.org/10.1007/s10569-006-9002-4
URI: 
Access Rights: 
Acesso restrito
Type: 
outro
Source:
http://repositorio.unesp.br/handle/11449/24846
Appears in Collections:Artigos, TCCs, Teses e Dissertações da Unesp

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