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

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Volume 695 (March 2025)

A&A, 695 (2025) C2

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202449383]

Table 2.

Mass-loss rate prescriptions from different works.

Ṁ relation (M_⊙ yr⁻¹)	DUSTY mode	Reference	Sample
$\dot{M} = 10^{- 8.158} L^{1.769} T_{eff}^{1.676}$ $\dot{M} = 10^{-8.158}L^{1.769}T_{\mathrm{eff}}^{1.676}$	–	de Jager et al. (1988)	Milky Way
$\dot{M} = 10^{- 5.56} {(\frac{L}{10^{4}})}^{1.05} {(\frac{T_{eff}}{3500})}^{- 6.3}$ $\dot{M}=10^{-5.56}\left(\frac{L}{10^4}\right)^{1.05}\left(\frac{T_{\mathrm{eff}}}{3500}\right)^{-6.3}$	RDW Analytic	van Loon et al. (2005)	LMC
$\dot{M} = 1.06 \times 10^{- 5} {(\frac{L}{10^{4}})}^{0.9} {(\frac{P}{500 d})}^{0.75} {(\frac{r_{gd}}{200})}^{- 0.03}$ $\dot{M}=1.06 \times 10^{-5}\left(\frac{L}{10^4}\right)^{0.9}\left(\frac{P}{500\,\mathrm{d}}\right)^{0.75}\left(\frac{r_{\mathrm{gd}}}{200}\right)^{-0.03}$	RDW	Goldman et al. (2017)	LMC
Analytic solution (see reference)	–	Kee et al. (2021)	–
log Ṁ = −21.5 − 0.15 M_ini+.36 log L	Steady-state, r⁻²	Beasor et al. (2023)	Galactic clusters
log Ṁ = 0.45(log L)³ − 5.26(log L)² + 20.93 log L −34.56	RDW	Yang et al. (2023)	SMC
$log \dot{M} = 0.26 log L - 14.19 log (\frac{T_{eff}}{4000}) - 9.17, log L < 4.4$ $\log{\dot{M}} = 0.26 \log{L}-14.19\log{\left(\frac{T_{\mathrm{eff}}}{4000}\right)} - 9.17, \ \log{L} < 4.4$	Steady-state, r⁻²	This work	LMC
$log \dot{M} = 2.5 log L - 33.7 log (\frac{T_{eff}}{4000}) - 19.1, log L ≳ 4.4$ $\log{\dot{M}} = 2.5 \log{L}-33.7\log{\left(\frac{T_{\mathrm{eff}}}{4000}\right)} - 19.1, \ \log{L} \gtrsim 4.4$

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