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

Author(s)
L. Decin, W. Homan, T. Danilovich, A. de Koter, D. Engels, L. B.F.M. Waters, S. Muller, C. Gielen, D. A. García-Hernández, R. J. Stancliffe, M. Van de Sande, G. Molenberghs, F. Kerschbaum, A. A. Zijlstra, I. El Mellah
Organisation(s)
Department of Astrophysics
External organisation(s)
Katholieke Universiteit Leuven, University of Leeds, University of Amsterdam (UvA), Universität Hamburg, SRON Netherlands Institute for Space Research , Chalmers University of Technology, University of La Laguna, University of Hull, University of Birmingham, Hasselt University, University of Manchester, Hong Kong Polytechnic University
Journal
Nature Astronomy
Volume
3
Pages
462-462
No. of pages
1
DOI
https://doi.org/10.1038/s41550-019-0761-8
Publication date
05-2019
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
ASJC Scopus subject areas
Astronomy and Astrophysics
Portal url
https://ucrisportal.univie.ac.at/en/publications/0b749535-01c5-4fc3-91e7-ce9923c7cca0