Physics
Scientific paper
Jan 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..349f&link_type=abstract
The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu
Physics
Scientific paper
Magnetohydrodynamic (MHD) simulations are presented for the long-term evolution of a stellar dipolar field connected to the surrounding accretion disk. As a main result, the initial large-scale dipole is destroyed and a two-component outflow evolves -- a stellar wind and a disk wind. This outflow is uncollimated and reaches velocities of about the Keplerian speed at its foot point.
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