Open Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202553799]


Issue
A&A
Volume 707, March 2026
Article Number C1
Number of page(s) 2
Section Stellar atmospheres
DOI https://doi.org/10.1051/0004-6361/202659227e
Published online 13 March 2026

In the original publication, the spectroscopic and evolutionary Eddington parameters were derived using the spectroscopic ΓespecMathematical equation: $\Gamma_{\rm e}^{\rm spec}$ and evolutionary ΓeevoMathematical equation: $\Gamma_{\rm e}^{\rm evo}$ masses, respectively. The values presented in Table A.1 were incorrect. All the values should be divided by a factor of two. This correction affects Fig. 12 (massloss rates log vs. Γe), Fig. 19 (wind efficiency parameter η vs. effective temperature Teff), Fig. 20 (ratio of the terminal wind velocity υ to the escape velocity υesc vs. Teff), and Eq. (8) in the original paper. We present the correct ΓespecMathematical equation: $\Gamma_{\rm e}^{\rm spec}$ and ΓeevoMathematical equation: $\Gamma_{\rm e}^{\rm evo}$ in Table 1 and the correct υesc,(1Γe)Mathematical equation: $\varv_{{\rm esc}, (1-\Gamma_{\rm e})}$ in Table 2.

Following these corrections to the parameters, some errors in the plots had to be corrected. Figure 12 of the original publication is replaced by Fig. 1, where the values of log Γe for the sample have been shifted leftward by -0.3 dex. Figures 19 and 20 in the original are replaced by Figs. 2 and 3, respectively. The colorbar labels in the original plots are shifted by -0.3 dex.

Equation (8) in the original is replaced by the following equation: υ/υesc=5.6(±1.0)log(Teff/K)22.3(±4.5).Mathematical equation: \varv_{\infty}/\varv_{\rm esc}=5.6(\pm 1.0)\log{(T_{\rm eff}/{\rm K})}-22.3(\pm 4.5).(1)

This correction also eliminates the issue with the abnormally high ΓespecMathematical equation: $\Gamma_{\rm e}^{\rm spec}$ and ΓeevoMathematical equation: $\Gamma_{\rm e}^{\rm evo}$ we obtained for our sample and the Γeevo>1Mathematical equation: $\Gamma_{\rm e}^{\rm evo} > 1$ we obtained for the hyper-giant Sk -68° 135, which was discussed in Sect. 4.3 of the original publication. It also brings our derived values more in line with the numerically predicted υesc from Krticka et al. (2024). These adjustments do not change the conclusions originally drawn from the study.


© The Authors 2026

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All Tables

Table 1

Correction to Table A.1 of the original publication.

Table 2

Correction to Table 3 of the original publication.

All Figures

Thumbnail: Fig. 1 Refer to the following caption and surrounding text. Fig. 1

Replacement of Fig. 12 of the original paper.

In the text
Thumbnail: Fig. 2 Refer to the following caption and surrounding text. Fig. 2

Replacement of Fig. 19 of the original paper.

In the text
Thumbnail: Fig. 3 Refer to the following caption and surrounding text. Fig. 3

Replacement of Fig. 20 of the original paper.

In the text

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