Clumping in [WC]-type Central Stars from electron-scattering line wings
H. Todt, W.-R. Hamann & G. Gräfener
While there is strong evidence for clumping in the winds of massive hot stars, very little is known about clumping in the winds from Central Stars. We have checked [WC]-type CSPN winds for clumping by inspecting the electron-scattering line wings. At least for three stars we found indications for wind inhomogeneities.
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