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• W1993034669 abstract "We present the results of an effort to model recent HST eclipse observations of the C IV 1550 Å resonance line in the high-inclination nova-like cataclysmic variable UX UMa. Assuming this line to be predominantly wind-formed, we are able to roughly reproduce the shapes and strengths of the observed line profiles (both away from and during eclipse) within the framework of a simple kinematic model in which the outflow is described as a rotating, biconical accretion disk wind. Our preferred model also matches most of the detailed behavior of different parts of the C IV line profile (blue wing, line center, and red wing) as a function of orbital phase." @default.
• W1993034669 created "2016-06-24" @default.
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• W1993034669 date "1997-09-01" @default.
• W1993034669 modified "2023-10-02" @default.
• W1993034669 title "Eclipse Mapping of the Accretion Disk Wind in the Cataclysmic Variable UX Ursae Majoris" @default.
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• W1993034669 doi "https://doi.org/10.1086/304519" @default.
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