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Table C.1

Best-fitting dX∕dQ values inferred for the single and binary SMC WR stars.

SMC d X∕d Q τH env Mmodel
AB [kyr] [M]
Single:
1 ≥ 35 ≤ 175 ≤ 0.56 32
2 18
4 22
9 30
10 20
11 26
12 28
Binary:
3 28
5 50
6 ≥ 16 ≤ 160 ≤ 0.58 50
7 34

Notes. Also displayed are the timescale on which the WR star would blow away its hydrogen-containing layers (τH env ) and the ratio of τH env to the helium burning timescale. The last column gives the best fitting current masses.

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