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Table 5

Bonnsai predictions for the current mass and lower limit for the age of VFTS 399.

log(Lbol/L) M curr Age
(M) (Myr)

4.7 ± 0.1 >
4.9 ± 0.1 >
5.2 ± 0.1 >

Notes. All four models utilise stellar temperature, surface gravity and projected equatorial rotational velocity as input parameters, while rows 24 present the results of including the stellar luminosity estimates (Col. 1) as an additional constraint. The quoted errors are 1σ uncertainties.

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