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Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction (vol 3, pg 408, 2019)

Tijdschriftbijdrage - Tijdschriftartikel

© 2019, Springer Nature Limited. 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.
Tijdschrift: Nature Astronomy
ISSN: 2397-3366
Issue: 5
Volume: 3
Pagina's: 462 - 462
Jaar van publicatie:2019