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.
The full article is available as PostScript file via anonymous ftp.
user: anonymous or ftp; Password: your e-mail address;
file: /usr/aftp/pub/wrhamann/workshop/todt.ps (410kB PostScript uncompressed)
or todt.ps.gz (120kB PostScript compressed)
or todt.pdf (90kB)