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Table 3

Initial parameters and ages derived from single-star tracks assuming inhomogeneous evolution for the primary.

Inhomogeneous primaries, single-star tracks

SMC AB  3 5 6 7 8

M1, i [M] a 50 100 80 70 80
Age [Myr]a 4.6 3.0 3.4 3.7 3.6
Rmax,1 [R] a 1800 1200 2000 2100 2000
Mi, 2 [M] b 15 100 46 35 50
vrot, i, 2[km s-1]b 230 170 160 130

–0.01 (0.03) –0.01 (0.05) –0.01 (0.06) –0.02 (0.04) 0.09 (0.15)
–0.08 (0.08) –0.04 (0.13) –0.16 (0.15) –0.07 (0.12) –0.09 (0.13)
2 (50) –13 (14) 8 (14) 8 (10)
–0.03 (0.05) −0.11 (0.05) −0.25 (0.1) –0.03 (0.05) 0.00 (0.05)

Notes. The upper part of the table gives the initial parameters and age defining the best-fitting single star tracks assuming a non-homogeneous evolution, as derived by the BPASS and BONNSAI tools, as well as the maximum radius reached by the primary throughout the evolution, Rmax,1. The lower part gives EnOn as obtained from the best-fitting BPASS track, along with corresponding σn values in parentheses (see Sect. 6.2). Underlined values denote deviations which exceed 2σ.

(a)

Obtained from the BPASS stellar evolution code;

(b)

obtained from the BONNSAI stellar evolution tool, except for AB 5, where the BPASS code was used (see text).

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