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2019NatAs...3..408D - Nature Astronomy, 3, 408-415 (2019)
Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction.
DECIN L., HOMAN W., DANILOVICH T., DE KOTER A., ENGELS D., WATERS L.B.F.M., MULLER S., GIELEN C., GARCIA-HERNANDEZ D.A., STANCLIFFE R.J., VAN DE SANDE M., MOLENBERGHS G., KERSCHBAUM F., ZIJLSTRA A.A. and EL MELLAH I.
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