The HARPS search for southern extra-solar planets - XIX. Characterization and dynamics of the GJ 876 planetary system

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Volume 511 (February 2010)

A&A, 511 (2010) A21

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Table 5:

Quasi-periodic decomposition of the resonant angle $\theta = 2 \lambda _b - \lambda _c - \varpi _2^*$ for an integration over 100 kyr of the orbital solution in Table 2.
Combination					$\nu_i$	A_i	$\phi_i$
n_b	n_c	g₂	g₃	$l_\theta$	(deg/yr)	(deg)	(deg)
0	0	0	0	1	245.9180	1.810	-48.681
1	1	-2	0	0	6586.5572	0.567	96.286
0	1	-1	0	0	2195.5191	0.569	32.095
0	0	-1	1	0	41.7516	0.411	-94.109
1	0	-1	0	0	4391.0382	0.255	-25.809
2	1	-3	0	0	10977.5954	0.156	-19.523
0	0	1	-1	1	204.1664	0.120	-44.572

Notes. We have $\theta = \sum_{i=1}^N A_i \cos(\nu_i~ t + \phi_i)$ . We only provide the first 7 largest terms that are identified as integer combinations of the fundamental frequencies given in Table 4.

Source LaTeX | All tables | In the text

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