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• W4297834224 endingPage "A114" @default.
• W4297834224 startingPage "A114" @default.
• W4297834224 abstract "Context. Low- and intermediate-mass stars go through a period of intense mass-loss at the end of their lives, during the asymptotic giant branch (AGB) phase. While on the AGB a significant part, or even most, of their initial mass is expelled in a stellar wind. This process controls the final stages of the evolution of these stars and contributes to the chemical evolution of galaxies. However, the wind-driving mechanism of AGB stars is not yet well understood, especially so for oxygen-rich sources. Characterizing both the present-day mass-loss rate and wind structure and the evolution of the mass-loss rate of such stars is paramount to advancing our understanding of this processes." @default.
• W4297834224 created "2022-10-01" @default.
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• W4297834224 date "2015-05-01" @default.
• W4297834224 modified "2023-10-14" @default.
• W4297834224 title "Dusty wind of W Hydrae" @default.
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• W4297834224 doi "https://doi.org/10.1051/0004-6361/201425092" @default.
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