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

    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.

    L. Decin, W. Homan, T. Danilovich, A. de Koter, D. Engels in Nature Astronomy (2019)

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    Article

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

    In 1981, the idea of a superwind that ends the life of cool giant stars was proposed1. Extreme oxygen-rich giants, OH/IR stars, develop superwinds with the highest mass-loss rates known so far, up to a few 10−4 s...

    L. Decin, W. Homan, T. Danilovich, A. de Koter, D. Engels in Nature Astronomy (2019)