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. 12.

Mass-loss rates vs. luminosity (left) and effective temperature (right) calculated from Eq. (1). The magenta points correspond to the prediction of the derived Ṁ(L,T_eff) relation, Eq. (7), showing the correlation of the mass-loss rate as a function of the luminosity and effective temperature.

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