Non-LTE effects strengthen the K I 7698 Å line, requiring abundance corrections up to -0.7 dex that align literature values with GCE models incorporating yields from rotating massive stars.
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Non-LTE analysis of K I in late-type stars
Non-LTE effects strengthen the K I 7698 Å line, requiring abundance corrections up to -0.7 dex that align literature values with GCE models incorporating yields from rotating massive stars.