Clumping in [WC]-type Central Stars from electron-scattering line wings

Physics

Scientific paper

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Scientific paper

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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