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A high-mass planetary nebula in a Galactic open cluster

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  1. Article

    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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