Fig. 4 from On the Velocity Structure in Clumpy Planetary Nebulae

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT 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. 4.

Terminal velocity is plotted as a function of normalized distance from the central star. The lower limit is the initial speed given by the internal postshock speed in the clumps, which is inversely proportional to the distance.

Other Images in This Article

Copyright and Terms & Conditions