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Paper: |
Link between Mass-Loss and Variability Type for AGB Stars? |
Volume: |
203, The Impact of Large-Scale Surveys on Pulsating Star Research, IAU Colloquium 176 |
Page: |
124 |
Authors: |
Ivezić, ž.; Knapp, G. R. |
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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