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. 14.

Effect of the grain size distribution on the mass-loss rate for a range of luminosities. Top: ratio of the mass-loss rates assuming an MRN grain size distribution in the range [0.01, 1] μm over the distribution in the range [0.1, 1] μm. Bottom: ratio of the minimum $χ_{mod}^{2}$ $\chi^2_{\rm mod}$ between the two mentioned cases.

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