Modeling of uv lines from cataclysmic variable winds

Conference · Sun Mar 01 04:00:00 EST 1992

OSTI ID:5399379

Vitello, P A ^[1]; Shlosman, I ^[2]

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1. Lawrence Livermore National Lab., CA (United States)
2. Kentucky Univ., Lexington, KY (United States). Dept. of Physics and Astronomy

Ultraviolet resonance lines appear to be powerful tools for diagnostics and study of the outflows from cataclysmic variable stars. The origin of these winds and their geometry are not known at present. In order to compare observed lines from the IUE database with synthetic line profiles from accretion disk winds, we have developed a numerical radiation transfer model for 3D non-radial, rotating winds from an accretion disk. Using this model we have studied line spectra from a number of cataclysmic variables. We find that good fits to be observed spectra can be obtained using disk winds for mass loss rates much smaller than the accretion rates.

• Research Organization: Lawrence Livermore National Lab., CA (United States)
• Sponsoring Organization: DOE; NASA; USDOE, Washington, DC (United States); National Aeronautics and Space Administration, Washington, DC (United States)
• DOE Contract Number: W-7405-ENG-48
• OSTI ID: 5399379
• Report Number(s): UCRL-JC-110303; CONF-9202103--2; ON: DE92013443; CNN: NAG5-1387
• Country of Publication: United States
• Language: English

Related Subjects

661300* -- Other Aspects of Physical Science-- (1992-)
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
DATA BASE MANAGEMENT
DIAGNOSTIC TECHNIQUES
MANAGEMENT
RADIATION TRANSPORT
SPECTRA
STAR ACCRETION
STAR EVOLUTION
STARS
STELLAR ACTIVITY
STELLAR WINDS
ULTRAVIOLET SPECTRA
VARIABLE STARS