Disk Winds in Cataclysmic Variables: from Numerical Simulations to Spectral Lines

Details Disk Winds in Cataclysmic Variables: from Numerical Simulations to Spectral Lines Disk Winds in Cataclysmic Variables: from Numerical Simulations to Spectral Lines

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.6301p&link_type=abstract

American Astronomical Society Meeting 204, #63.01; Bulletin of the American Astronomical Society, Vol. 36, p.776

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Scientific paper

We report on resonance-line profiles predicted by radiation-driven disk-wind models. The line profiles reproduce very well the line absorption of the nova-like variable IX Vel and promise to reproduce observations of other cataclysmic variables. This success of the radiation-driven disk-wind model provides an important link between outflows in OB stars and outflows in active galactic nuclei.
We acknowledge support from NASA grant NAG5-11736.

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