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On the Velocity Structure in Clumpy Planetary Nebulae
Steffen & López 2004 The Astrophysical Journal 612 319.
Caption: Fig. 7.
Logarithmic density is shown for RUN 1 after (a) 44.2 and (b) 116.7 yr.
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© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.