The EUV Emission-Line Spectrum of OY Carinae in Superoutburst: Scattering in the Wind

Details The EUV Emission-Line Spectrum of OY Carinae in Superoutburst: Scattering in the Wind The EUV Emission-Line Spectrum of OY Carinae in Superoutburst: Scattering in the Wind

May 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000rmxac...9..232m&link_type=abstract

"Astrophysical Plasmas: Codes, Models, and Observations, Proceedings of the conference held in Mexico City, October 25-29, 1999,

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Extreme Ultraviolet Explorer/ satellite observed the cataclysmic variable OY Carinae in superoutburst for 3 days in 1997 March. The resulting 80-180 Å spectrum, which contains broad (FWHM~ 2000 km s-1) emission lines of O V-O VI, Ne V-Ne VI, Mg V-Mg VI and Fe VI-Fe VIII, is well modeled by scattering of boundary layer radiation in the system's accretion disk wind.

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