Author Correction: Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction

Bibcode
2019NatAs...3..462D
DOI
10.1038/s41550-019-0761-8
Muller, S.; Gielen, C.; Waters, L. B. F. M.; Engels, D.; Danilovich, T.; de Koter, A.; Decin, L.; Homan, W.; García-Hernández, D. A.; Stancliffe, R. J.; Van de Sande, M.; Molenberghs, G.; Kerschbaum, F.; Zijlstra, A. A.; El Mellah, I.
Bibliographical reference

Nature Astronomy, Volume 3, p. 462-462

Advertised on:
3
2019
Number of authors
15
IAC number of authors
1
Citations
2
Refereed citations
2
Description
In the version of this Letter originally published, the caption of Fig. 2 incorrectly said J = 3-2; it should have said J = 2-1. This has now been corrected.
Type
Erratum

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