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Link between Mass-Loss and Variability Type for AGB Stars?
Published online by Cambridge University Press: 12 April 2016
Abstract
We discuss difficulties in explaining the distribution of AGB stars in the 25–12 vs. 12–K color–color diagram by steady-state radiatively driven models, and propose that the discrepancy may be due to changes of mass-loss rate with the time scales of ∼ 100 yr.
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- Part 2. Variability of High-Luminosity Stars
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- Copyright © Astronomical Society of the Pacific 2000
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