ASPCS
 
Back to Volume
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.
Back to Volume