| Issue |
A&A
Volume 641, September 2020
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 2 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201935684e | |
| Published online | 03 September 2020 | |
The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud
Spectroscopy, orbital analysis, formation, and evolution (Corrigendum)
1
Institute of Astrophysics, KU Leuven, Celestijnlaan 200D, 3001 Leuven, Belgium
e-mail: tomer.shenar@kuleuven.be
2
Leibniz-Institut für Astrophysik Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
3
Institut für Physik und Astronomie, Universität Potsdam, Karl-Liebknecht-Str. 24/25, 14476 Potsdam, Germany
4
Département de physique and Centre de Recherche en Astrophysique du Québec (CRAQ), Université de Montréal, 6128, Succ. Centre-Ville, Montréal, Québec H3C 3J7, Canada
5
Armagh Observatory, College Hill, BT61 9DG Armagh, UK
6
Cherenkov Telescope Array Observatory gGmbH, Via Piero Gobetti 93/3, 40126 Bologna, Italy
7
Astronomy and Astrophysics Research Group, Vrije Universiteit Brussel, Pleinlaan 2, 1050 Brussels, Belgium
8
The observatories of the Carnegie institution for science, 813 Santa Barbara St., Pasadena, CA 91101, USA
This article has no abstract.
Key words: stars: massive / stars: Wolf-Rayet / Magellanic Clouds / binaries: close / binaries: spectroscopic / errata, addenda
© ESO 2020
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