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- W3185725307 abstract "Abstract As evidenced by the P Cygni profiles of their ultraviolet resonance lines, cataclysmic variables—like early-type stars—are known to have extensive, high velocity winds. Assisted by AAVSO visual data and IUE ultraviolet spectra, we present an observational and theoretical study of the P Cygni profiles of the dwarf nova HL CMa. As these profiles are dependent upon the ionization structure of the wind, we describe a model of a radiatively-driven shocked wind for cataclysmic variables, and present results for the temperature and ionization structure of the outflowing gas." @default.
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- W3185725307 date "1987-01-01" @default.
- W3185725307 modified "2023-09-25" @default.
- W3185725307 title "IUE Observations of HL CMa and the Winds of Cataclysmic Variables" @default.
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- W3185725307 doi "https://doi.org/10.1017/s0252921100104968" @default.
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