Macroclumping, Magnetic Fields, and X-Rays in Massive Stars
Lidia Oskinova, Wolf-Rainer Hamann, Helge Todt, Andreas Sander
Modern stellar wind models should account for new effects that were traditionally ignored in classical model atmospheres. Among these effects are stellar magnetic fields, X-ray emission, and wind clumping. The X-rays strongly affect the ionization structure of the winds. In O-type supergiants, clumping must be accounted for in the models to derive correct stellar parameters from X-ray or UV spectroscopy
The article is available via anonymous ftp.
Server: ftp.astro.physik.uni-potsdam.de
user: anonymous or ftp; Password: your e-mail address;
cd pub/wrhamann
files: as in the links listed below
WEB link:
oskinova-canada2011.pdf (600 kB)