The effect of grain drift on the structure of (Post-) AGB winds

Details The effect of grain drift on the structure of (Post-) AGB winds The effect of grain drift on the structure of (Post-) AGB winds

1999-09-29

arxiv.org/abs/astro-ph/9909490v1

Astronomy and Astrophysics

Astrophysics

To appear in "Asymmetrical Planetary Nebulae II: from Origins to Microstructures" ASP Conference Series, J.H. Kastner, N. Soke

Scientific paper

We have developed an implementation for the momentum transfer force in numerical two fluid hydrodynamics. This form of the frictional coupling between gas and grains is consistent with the microscopic interactions between the two components. The coupling force gives rise to a drift velocity of the grains with respect to the gas. We apply this mechanism to the outflow of (Post-) AGB objects. Our numerical hydrodynamics code calculates self consistently the dynamics of these outflows, as well as the nucleation and growth of grains and equilibrium chemistry of the gas. Grain nucleation and growth are processes that depend strongly on the rate of gas-grain collisions. Hence, the drift velocity becomes an important variable. The tight connection between grain chemistry and drift causes the system to become extremely sensitive to small changes in almost any parameter. This may be a cause for deviation from (spherical) symmetry and structure.

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