Dynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12

Callegari, N.FerrazMello, S.Michtchenko, T. A.2014-02-262014-05-202014-02-262014-05-202006-04-01Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 94, n. 4, p. 381-397, 2006.0923-2958http://hdl.handle.net/11449/24846This 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.381-397engchaosextra-solar planetsplanetary systemspulsar planetsresonanceDynamics of two planets in the 3/2 mean-motion resonance: Application to the planetary system of the pulsar PSR B1257+12Artigo10.1007/s10569-006-9002-4WOS:000238517200002Acesso restrito