Dynamics of Two Planets in the 3/2 Mean-motion Resonance: Application to the Planetary System of the Pulsar PSR B1257+12-Reference-Cited by-同舟云学术

Dynamics of Two Planets in the 3/2 Mean-motion Resonance: Application to the Planetary System of the Pulsar PSR B1257+12

Published:2006-04 Issue:4 Volume:94 Page:381-397
ISSN:0923-2958
Container-title:Celestial Mechanics and Dynamical Astronomy
language:en
Short-container-title:Celestial Mech Dyn Astr

Author:

Callegari N.,Ferraz-Mello S.,Michtchenko T. A.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics,Applied Mathematics,Computational Mathematics,Mathematical Physics,Modeling and Simulation

Link

http://link.springer.com/content/pdf/10.1007/s10569-006-9002-4.pdf

Reference24 articles.

1. Beaugé C., Callegari N. Jr., Ferraz-Mello S., Michtchenko T.A. Resonances and stability of extra-solar planetary systems. In: Z. Knežević and A. Milani (eds.) IAU Colloq. 197, 3–18 (2005)

2. Callegari Jr., N. Ressonâncias 2:1 e 3:2 em sistemas planetários. Dr. Thesis, Univ. Sao Paulo, SP (2003)

3. Callegari Jr., N., Michtchenko, T.A., Ferraz-Mello, S. Dynamics of two planets in resonances: the 2:1, 3:2 and 5:2 cases. Inst. Appl. Astron. RAS, Transactions. 8, 47–52 (2002)

4. Callegari N. Jr., Michtchenko T.A., Ferraz-Mello S. (2004) Dynamics of two planets in the 2/1 mean-motion resonance. Celest. Mech. Dyn. Astr. 89, 201–234

5. Ferraz-Mello S., Michtchenko T.A. (2002) Extra-solar planetary system. Rev. Mex. A. A. Conf. Ser. 14, 7–10

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