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- W201549995 abstract "High-resolution infrared spectroscopy of molecular lines provides a powerful diagnostic probe to investigate the spatial structure and temporal evolution of the cool, dusty winds of Miras and long—period variables, such as the carbon rich IR-Mira IRC+10216 (Keady et al. 1988). For this object, high-resolution spectra of the CO fundamental and first overtone transitions at 5μm and 2μm have been obtained repeatedly over an interval spanning more than ten years. The unsaturated overtone lines reflect the actual conditions and their temporal changes in the acceleration region of the wind. The line profiles show a multi-component absorption structure, and spectra from different epochs reveal changes of the line profiles (e.g., the emergence of a new absorption component) on time scales that are much longer than the period of the star (Sada 1993)." @default.
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- W201549995 date "1998-01-01" @default.
- W201549995 modified "2023-10-02" @default.
- W201549995 title "Temporal Variations of CO Infrared Lines in Cool-Star Winds" @default.
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- W201549995 doi "https://doi.org/10.1007/978-3-540-68597-5_71" @default.
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