A statistical test on the reliability of the non-coevality of stars in binary systems

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Volume 587 (March 2016)

A&A, 587 (2016) A31

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Table A.1

Critical values W_0.95 in dependence on masses of the stars M₁ and M₂ (both in solar units), and on their initial metallicity [Fe/H].


M₁	[Fe/H]	M₂
		0.8	0.9	1.0	1.1	1.2	1.3	1.4	1.5	1.6


0.80	–0.55	0.591
0.90	–0.55	0.643	0.561
1.00	–0.55	0.625	0.595	0.517
1.10	–0.55	0.617	0.603	0.581	0.536
1.20	–0.55	0.683	0.692	0.641	0.620	0.545
1.30	–0.55		0.786	0.741	0.667	0.611	0.588
1.40	–0.55		0.816	0.763	0.663	0.617	0.594	0.579
1.50	–0.55			0.792	0.695	0.601	0.594	0.587	0.568
1.60	–0.55				0.692	0.564	0.554	0.582	0.605	0.472


0.80	–0.25	0.598
0.90	–0.25	0.662	0.585
1.00	–0.25	0.661	0.629	0.572
1.10	–0.25	0.629	0.606	0.603	0.534
1.20	–0.25	0.623	0.619	0.613	0.603	0.507
1.30	–0.25		0.726	0.699	0.688	0.614	0.539
1.40	–0.25			0.779	0.734	0.682	0.593	0.574
1.50	–0.25			0.796	0.740	0.676	0.592	0.574	0.562
1.60	–0.25				0.732	0.650	0.582	0.576	0.601	0.458


0.80	0.00	0.602
0.90	0.00	0.659	0.603
1.00	0.00	0.673	0.645	0.598
1.10	0.00	0.681	0.637	0.628	0.588
1.20	0.00	0.702	0.648	0.615	0.610	0.541
1.30	0.00		0.686	0.623	0.628	0.604	0.518
1.40	0.00			0.730	0.696	0.674	0.618	0.535
1.50	0.00			0.806	0.767	0.710	0.677	0.571	0.544
1.60	0.00				0.774	0.688	0.670	0.592	0.594	0.455


0.80	0.25	0.625
0.90	0.25	0.683	0.618
1.00	0.25	0.678	0.660	0.620
1.10	0.25	0.678	0.654	0.648	0.608
1.20	0.25	0.708	0.658	0.630	0.633	0.584
1.30	0.25		0.717	0.644	0.632	0.606	0.535
1.40	0.25			0.688	0.631	0.616	0.577	0.534
1.50	0.25			0.769	0.713	0.674	0.632	0.595	0.510
1.60	0.25				0.780	0.729	0.677	0.661	0.586	0.445


0.80	0.55	0.643
0.90	0.55	0.693	0.644
1.00	0.55	0.687	0.671	0.630
1.10	0.55	0.671	0.653	0.659	0.620
1.20	0.55	0.715	0.653	0.649	0.647	0.604
1.30	0.55		0.699	0.643	0.633	0.630	0.580
1.40	0.55		0.731	0.659	0.611	0.630	0.626	0.495
1.50	0.55			0.708	0.643	0.592	0.601	0.537	0.421
1.60	0.55			0.748	0.685	0.612	0.610	0.619	0.559	0.281

Notes. Values are computed for primary relative age r = 0.1.

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