Image Details

Choose export citation format:

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. 12.

Logarithm of the number density is shown for the slab symmetric simulation C32 at a time of about 8 cloud‐crushing times ﹩t_{\mathrm{cc}\,}﹩ (﹩3.45\times 10^{9}﹩ s) after the beginning of the interaction; ﹩t_{\mathrm{cc}\,}﹩ is the time to maximum compression of the unfragmented cloud after the beginning of the interaction.

Other Images in This Article

Show More

Copyright and Terms & Conditions