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- W1636691873 abstract "We evaluate the accuracy with which the properties of late-type giant star winds can be estimated by fitting ultraviolet line profiles and radio continuum emission. Our test cases include the stars α TrA (K4 II), λ Vel (K4 Ib-II), and ζ Aur (K4 Ib + B5 V). Of particular interest is the sensitivity of the line profiles to the wind parameters Ṁ, v ∞, v turb, β, and T wind. We are finding that while accurate and reliable values of Ṁ are difficult to obtain, the most reliable values come from the application of two or more independent techniques.KeywordsSolar WindRadio EmissionOrbital PhaseAlfven WaveRadio FluxThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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- W1636691873 date "1998-01-01" @default.
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- W1636691873 title "A Critical Evaluation of Mass-Loss Rates and Wind Properties of Evolved Late-Type Stars" @default.
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- W1636691873 doi "https://doi.org/10.1007/978-3-540-68597-5_5" @default.
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