Calibrating convective-core overshooting with eclipsing binary systems - The case of low-mass main-sequence stars

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Volume 587 (March 2016)

A&A, 587 (2016) A16

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Table 4

Same as Table 3, but only for the impact of α_ml and diffusion efficiency, restricting the mass range of the secondary stars to M₂> 1.4M_⊙ and M₂> 1.5M_⊙.

Primary star relative age
	0.0	0.1	0.2	0.3	0.4	0.5	0.6	0.7	0.8	0.9	1.0

M₂ > 1.4 M_⊙

Unknown mixing-length value
q_0.025	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.07
q_0.16	0.03	0.04	0.04	0.03	0.03	0.03	0.03	0.03	0.03	0.07	0.15
	0.12	0.15	0.15	0.12	0.14	0.17	0.19	0.17	0.15	0.17	0.19
	0.15	0.17	0.16	0.17	0.17	0.20	0.19	0.20	0.17	0.23	0.24
q _0.84	0.33	0.32	0.30	0.34	0.35	0.38	0.38	0.36	0.38	0.34	0.30
q _0.975	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40

Unknown element diffusion efficiency
q _0.025	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.09
q _0.16	0.04	0.05	0.04	0.03	0.03	0.03	0.03	0.03	0.03	0.07	0.15
	0.15	0.15	0.16	0.17	0.17	0.17	0.19	0.20	0.17	0.20	0.17
	0.15	0.15	0.18	0.20	0.24	0.28	0.30	0.28	0.28	0.20	0.20
q _0.84	0.34	0.30	0.32	0.35	0.38	0.38	0.39	0.38	0.38	0.38	0.28
q _0.975	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.36

M₂> 1.5 M _⊙

Unknown mixing-length value
q _0.025	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.10
q _0.16	0.03	0.03	0.03	0.02	0.03	0.03	0.03	0.03	0.03	0.07	0.15
	0.13	0.15	0.14	0.10	0.12	0.17	0.17	0.17	0.11	0.16	0.20
	0.17	0.17	0.16	0.20	0.21	0.20	0.20	0.20	0.17	0.21	0.23
q _0.84	0.33	0.30	0.31	0.35	0.38	0.38	0.38	0.38	0.38	0.33	0.30
q _0.975	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.39

Unknown element diffusion efficiency
q _0.025	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.00	0.10
q _0.16	0.04	0.05	0.03	0.03	0.03	0.03	0.03	0.03	0.03	0.05	0.15
	0.15	0.15	0.14	0.20	0.21	0.19	0.17	0.20	0.11	0.17	0.18
	0.17	0.16	0.20	0.24	0.27	0.28	0.33	0.30	0.30	0.17	0.20
q _0.84	0.33	0.30	0.35	0.38	0.38	0.38	0.39	0.38	0.38	0.35	0.25
q _0.975	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.40	0.35

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