Issue |
A&A
Volume 676, August 2023
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|
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Article Number | C3 | |
Number of page(s) | 1 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201525645e | |
Published online | 04 August 2023 |
Wind mass transfer in S-type symbiotic binaries
II. Indication of the wind focusing (Corrigendum)
Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, Slovakia
e-mail: nshagatova@ta3.sk
Key words: binaries: symbiotic / stars: mass-loss / stars: winds / outflows / errata / addenda
We report an erratum to Shagatova et al. (2016). Due to the incorrect reasoning, Eqs. (17) and (18) contain redundant factor 2, leading to two times higher values of the spherical equivalent of the mass-loss rate Ṁsp in Table 3. However, the conclusions of the original article remain valid since the correct values of Ṁsp are of the same order of ≈10−6 M⊙ yr−1 for typical terminal velocities of the red giant wind in symbiotic systems. We apologize for any inconvenience that may have been caused due to our error. In the paragraph below, the revised version of Sect. 4.2 is given, except for its first and last sentence, which are correct, in addition to Table 3 with proper values of Ṁsp.
For the integral (5) expressed in the length units of RG, we can rewrite Eq. (9) as
Then, using Eq. (6) we obtain the relationship
where n1 is the resulting parameter of our models (see Table 2).
© The Authors 2023
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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