Volume 647, March 2021
|Number of page(s)||1|
|Section||Stellar structure and evolution|
|Published online||29 March 2021|
Exploring velocity limits in the thermonuclear supernova ejection scenario for hypervelocity stars and the origin of US 708 (Corrigendum)
Max Planck Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85748 Garching bei München, Germany
2 University of Leicester, University Road, LE1 7RH Leicester, Leicestershire, UK
Key words: binaries: close / supernovae: general / subdwarfs / white dwarfs / errata / addenda
Due to a typographical error in Table B.1, line three of the third column was reproduced in line four of the fourth column when that space should have been left blank. The corrected table is given as follows:
Parameters used in Eqs. (B.2)–(B.4).
© P. Neunteufel 2021
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.
Open Access funding provided by Max Planck Society.
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