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Formation and evolution of the two 4/3 resonant giants planets in HD 200964
Astronomy and Astrophysics
It has been suggested that HD 200964 is the first exoplanetary system with two Jovian planets evolving in the 4/3 mean- motion resonance. Previous scenarios to simulate the formation of two giant planets in the stable 4/3 resonance configuration have failed. Moreover, the orbital parameters available in the literature point out an unstable configuration of the planetary pair. The purpose of this paper is i) to determine the orbits of the planets from the RV measurements and update the value ofdoi:10.1051/0004-6361/201424820 fatcat:wr43dkopr5hmfpgbuitm5lljfe