An absence of binary companions to Wolf-Rayet stars in the Small Magellanic Cloud - Implications for mass loss and black hole masses at low metallicities

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Volume 689 (September 2024)

A&A, 689 (2024) A157

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Table B.2.

Same as Table B.1, but instead of only considering circular orbits we consider eccentric orbits with eccentricities that are drawn from a flat distribution between 0 and 0.9.

	$\hat{p}$ $\hat{p}$	${\hat{p}}_{M 5 +}$ $\hat{p}_{\mathrm{M5+}}$	${\hat{p}}_{P 1 yr -}$ $\hat{p}_{\mathrm{P1yr-}}$	${\hat{p}}_{M 5 + P 1 yr -}$ $\hat{p}_{\mathrm{M5+P1yr-}}$	${\hat{p}}_{P 30 d +}$ $\hat{p}_{\mathrm{P30d+}}$	${\hat{p}}_{L 20}$ $\hat{p}_{\mathrm{L20}}$	${\hat{p}}_{L 20, P 30 d +}$ $\hat{p}_{\mathrm{L20,P30d+}}$	${\hat{p}}_{R 19}$ $\hat{p}_{\mathrm{R19}}$	${\hat{p}}_{R 19, P 30 d +}$ $\hat{p}_{\mathrm{R19,P30d+}}$

M₂ restr.		M₂ > 5		M₂ > 5
1P_orb restr.			P_orb < 1 yr	P_orb < 1 yr	P_orb > 30 d		P_orb > 30 d		P_orb > 30 d
SMC AB1	0.847	0.895	0.943	0.980	0.756	0.948	0.937	0.950	0.918
SMC AB2	0.911	0.946	0.970	0.991	0.853	0.978	0.973	0.977	0.963
SMC AB4	0.889	0.931	0.959	0.987	0.822	0.969	0.963	0.970	0.951
SMC AB9	0.856	0.895	0.955	0.984	0.769	0.966	0.960	0.946	0.913
SMC AB10	0.941	0.960	0.991	0.998	0.901	0.994	0.993	0.984	0.973
SMC AB11	0.870	0.908	0.959	0.985	0.790	0.964	0.956	0.955	0.926
SMC AB12	0.831	0.874	0.941	0.976	0.729	0.945	0.933	0.933	0.890
Average	0.878	0.916	0.960	0.986	0.803	0.966	0.968	0.959	0.933

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