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A wind nebula generating extended X-ray emission was recently detectedsurrounding Swift 1834.9-0846. This is the first magnetar for which such a(pulsar) wind nebula (PWN) was found. I demonstrate that Swift 1834.9-0846'snebula can be rotationally-powered if it is being compressed by theenvironment. The physical reason behind this is the dominance of adiabaticheating over all other cooling and escape processes. This effect can happenonly for pulsars of relatively low spin-down power and can make for veryefficient nebulae. This contribution is based on previous work published in ApJ835, article id. 54, 13 pp. (2017).

Magnetar nebulae can be rotationally powered