Migration of planets in circumbinary discs | Astronomy & Astrophysics (A&A)

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Table 5

Final orbital parameters of the embedded planets using the observed m_p for the five systems investigated, calculated using the PLUTO simulations.

System	a_p [a_bin]	a_obs [a_bin]	e_p	e_obs
Kepler-16	4.18	3.20	0.03	0.00685
Kepler-34	7.77	4.74	0.31	0.182
Kepler-35	4.47	3.35	0.12	0.042
Kepler-38	3.98	3.10	0.02	0.032
Kepler-413	5.53	3.55	0.30	0.1181

Notes. The observed data are displayed also, for comparison. The semi-major axis (a_p) and eccentricity (e_p) of the planets are obtained through time averages over several thousand binary orbits at the end of the simulations.

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