TY  - CHAP
A1  - Todt, Helge Tobias
A1  - Hamann, Wolf-Rainer
A1  - Gräfener, G.
T1  - Clumping in [WC]-type Central Stars from electron-scattering line wings
N2  - 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.
Y1  - 2007
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus-17711
ER  -