Keywords :
hydrodynamics - stars winds, outflows - stars: carbon - stars: circumstellar matter - stars: mass-loss - stars: AGB and post-AGB
Abstract:In order to investigate the relations between the mass loss from pulsating red giants and quantities which can be obtained from observations, we have explored the behavior of theoretical models which treat the time-dependent hydrodynamics of circumstellar outflows, including a detailed treatment of the dust formation process. This approach, while ignoring effects such as a possible non-sphericity of the stellar atmospheres which are difficult to assess, accounts correctly for factors such as the grain formation and destruction which are crucial to the mass-loss mechanism. We built a grid of ~150 models covering a wide range of physical situations. This grid allows us to characterize the effects of different parameters,
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