Clumpy Flows in Protoplanetary and Planetary Nebulae
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Many astrophysical flows occur in inhomogeneous media. We briefly discuss some general properties of the adiabatic and radiative inhomogeneous systems and discuss the relevance of those properties to the planetary nebulae systems. We then focus on radiative hypersonic bullets and the applicability of this model to planetary and protoplanetary systems such as CRL 618, NGC 6543, Hen 3-1475.
4 pages, 2 figures. To appear in "Asymmetric Planetary Nebulae III", eds. M. Meixner, J. Kastner, N. Soker and B. Balick, 2004, ASP Conference Series, for higher resolution version and animations see http://www.pas.rochester.edu/~wma
4 pages, 2 figures. To appear in "Asymmetric Planetary Nebulae III", eds. M. Meixner, J. Kastner, N. Soker and B. Balick, 2004, ASP Conference Series, for higher resolution version and animations see http://www.pas.rochester.edu/~wma