Intermittent transition to irregular pulsation with mass loss in hydrodynamic models

@inproceedings{Aikawa1988IntermittentTT,
  title={Intermittent transition to irregular pulsation with mass loss in hydrodynamic models},
  author={Toshiki Aikawa},
  year={1988}
}
Introduction Hydrodynamic simulations of non-linear pulsation for less-massive cooler supergiants have been perfoemed by several authors (Tuchman, Sack and Barkat, 1979; Fadeyev and Tutukov, 1981; Fadeyev, 1982, 1984; Nakata, 1987; Buchler et al., 1987). The outburst of large amplitude pulsation at times is one of common features of these models, and renders mass-loss from the atmosphere of pulsating stars by generating strong shock waves. Models and resuits To find out routes of the transition… CONTINUE READING