Fig. 12

Possible secular trajectories for the KOI-1257 system seen in the (ω,i) plane
(top), and in the (ω,ein) plane
(bottom). The colours are preserved in both pictures, each one
corresponding to the same orbital evolution. The trajectories correspond to the
level curves of constant energy using the quadrupolar approximation combined with
general relativity. The dashed lines define the regions of initial conditions that
are compatible with the observational data (Table 6), namely ° (top) and
ein =
0.772 (bottom), while 105° ≤ ω ≤
177°
(Eqs. (8)−(10)).
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