Determining stellar properties of massive stars in NGC346 in the SMC with a Bayesian statistic technique

Open Access

Fig. 3

Violin plot of sampler RV returns for each MUSE observation of SSN 62. This is an example of an SB1 as at least two median RVs have a separation of >10 km s⁻¹ and the RV differences in two epochs is significant with a separation >4σ.

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