Bonnsai predictions for the current mass and lower limit for the age of VFTS 399.
|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 2−4 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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