The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: Spectroscopy, orbital analysis, formation, and evolution (Corrigendum)

T. Shenar, D. P. Sablowski, R. Hainich, H. Todt, AFJ Moffat, L.~M. Oskinova, V. Ramachandran, H Sana, A. A. C. Sander, O. Schnurr, N. St-Louis, Dany Vanbeveren, Y. Götberg, W.-R. Hamann

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

Abstract

The mass-loss rates Ṁ provided for the Wolf-Rayet (WR) stars in Table 2 in the original paper were derived from the transformed radii Rt. While Rt is correctly defined in the paper (Eq. (2)), an incorrect exponent was implemented in the script used to calculate them (3/2 instead of 2/3). As a consequence, the Ṁ values, Fig. 22, and the coefficients given in Table 5 in the original paper for the Ṁ relations (Eq. (6)) are impacted. Tables 1 and 2 in this corrigendum list the revised values, and Fig. 1 shows the revised version of Fig. 22 in the original paper. Moreover, a typo pertaining to the Rt value of BAT99 119 is corrected.
Original languageEnglish
Article numberC2
Number of pages2
JournalAstronomy & Astrophysics
Volume641
DOIs
Publication statusPublished - 3 Sep 2020

Fingerprint

Dive into the research topics of 'The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: Spectroscopy, orbital analysis, formation, and evolution (Corrigendum)'. Together they form a unique fingerprint.

Cite this