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


Issue
A&A
Volume 695, March 2025
Article Number C2
Number of page(s) 1
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/202554263e
Published online 18 March 2025

We found a typographical mistake in Tables 3 and 4 of our original paper where we presented the coefficients of our mass-loss rate relation. More specifically, the values of c2 and c3 for log(L/L)≳4.4 were the ones for steady-state winds and the MRN grain size distribution in the range of [0.01, 1] μm instead of [0.1, 1], which is presented in our main results.

1. Results

Tables 1 and 2 are the corrected versions of Tables 3 and 4, respectively, appearing in our paper but replaced with the corrected values for c2 and c3 at log(L/L)≳4.4 for our relation:

log M ˙ = c 1 log L + c 2 log ( T eff 4000 ) + c 3 . $$ \begin{aligned} \log {\dot{M}} = c_1 \log {L} + c_2\log {\left(\frac{T_{\rm eff}}{4000}\right)} + c_3. \end{aligned} $$(1)

Table 1.

Best-fit parameters of Eq. (1).

Table 2.

Mass-loss rate prescriptions from different works.

2. Conclusion

The figures and conclusions of our work remain the same, since the mistake was just a typo.

Acknowledgments

We thank Amedeo Romagnolo for bringing this mistake to our attention.

References

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© The Authors 2025

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All Tables

Table 1.

Best-fit parameters of Eq. (1).

Table 2.

Mass-loss rate prescriptions from different works.

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