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On the Velocity Structure in Clumpy Planetary Nebulae

  • Authors: W. Steffen and J. A. López

Steffen & López 2004 The Astrophysical Journal 612 319.

  • Provider: AAS Journals

Caption: Fig. 2.

For two different values of η and five values of initial distances we have plotted the velocity of clumps as a function of normalized distance. The curves are connected among each other by isolines of normalized time. Given the time delay in the arrival of the global shock at the different positions, the initial isotime line does not include all clumps. The initial normalized internal cloud shock velocities where ﹩\overline{v}_{cs}=0.2( \eta \overline{r}_{0}) ^{-1}﹩.

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