The main evolutionary pathways of massive hierarchical triple stars

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Volume 678 (October 2023)

A&A, 678 (2023) A60

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Table A.1.

Normalised incidence rates of evolutionary channels for all population models. The 3σ errors are based on Poisson uncertainties obtained by bootstrapping of the data

	Inner MT	Tertiary MT	Inner Orbit Unbound	Outer Orbit Unbound	Non-Interacting	Dynamical Destabilisation
Fiducial	0.673 ± 0.009	0.018 ± 0.003	0.100 ± 0.006	0.189 ± 0.008	0.002 ± 0.001	0.017 ± 0.002
a_in-Sana	0.734 ± 0.009	0.024 ± 0.003	0.059 ± 0.004	0.168 ± 0.007	0.002 ± 0.001	0.013 ± 0.002
a_out-Sana	0.687 ± 0.009	0.024 ± 0.003	0.088 ± 0.005	0.180 ± 0.007	0.002 ± 0.001	0.019 ± 0.003
a_in & a_out-Sana	0.751 ± 0.008	0.032 ± 0.003	0.051 ± 0.004	0.150 ± 0.007	0.004 ± 0.001	0.016 ± 0.002
e_in-Sana	0.644 ± 0.009	0.026 ± 0.003	0.115 ± 0.006	0.196 ± 0.007	0.004 ± 0.001	0.016 ± 0.002
e_out-Sana	0.646 ± 0.009	0.014 ± 0.002	0.116 ± 0.006	0.195 ± 0.008	0.004 ± 0.001	0.026 ± 0.003
e_in-flat	0.661 ± 0.009	0.025 ± 0.003	0.105 ± 0.006	0.192 ± 0.007	0.004 ± 0.001	0.015 ± 0.002
e_out-flat	0.659 ± 0.009	0.015 ± 0.002	0.107 ± 0.006	0.192 ± 0.008	0.004 ± 0.001	0.023 ± 0.003
q_out-Moe	0.766 ± 0.008	0.004 ± 0.001	0.137 ± 0.007	0.069 ± 0.005	0.001 ± 0.001	0.022 ± 0.003
i_rel-const	0.646 ± 0.009	0.025 ± 0.003	0.107 ± 0.006	0.200 ± 0.007	0.004 ± 0.001	0.018 ± 0.003

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