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), University of Hamburg, SRON Netherlands Institute for Space Research , Chalmers University of Technology, University of La Laguna, University of Hull, University of Birmingham, University of Manchester, Hong Kong Polytechnic University, Hasselt University
- Journal
- Nature Astronomy
- Volume
- 3
- Pages
- 408-415
- No. of pages
- 8
- DOI
- https://doi.org/10.1038/s41550-019-0703-5
- Publication date
- 05-2019
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103003 Astronomy, 103004 Astrophysics
- Keywords
- ASJC Scopus subject areas
- Astronomy and Astrophysics
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/acf41161-066b-44f8-8e22-b391401614dd