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

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

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006cemda..94..381c&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, Volume 94, Issue 4, pp.381-397

Astronomy and Astrophysics

Astronomy

6

Chaos, Extra-Solar Planets, Planetary Systems, Pulsar Planets, Resonance

Scientific paper

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.

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