Establishing a mass-loss rate relation for red supergiants in the Large Magellanic Cloud

Open Access

This article has an erratum: [https://doi.org/10.1051/0004-6361/202554263e]

Fig. 6.

Distributions of SED fitting parameters. Left: distribution of the minimum $χ_{mod}^{2}$ $\chi^2_{\rm mod}$ . The vertical lines show the σ_χ² (green dotted) and the 3σ_χ² (dashed orange) limits. Right: distribution of the best-fit optical depth, τ_V. Orange indicates τ_V from models with $χ_{mod}^{2} < 3 σ_{χ^{2}}$ $\chi^2_{\rm mod}<3\sigma_{\chi^2}$ .

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