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2003ApJ...597L..53Y - Astrophys. J., 597, L53-L56 (2003/November-1)
A model for the formation of high-density clumps in proto-planetary nebulae.
YOUNG P.A., HIGHBERGER J.L., ARNETT D. and ZIURYS L.M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Astrochemistry - Hydrodynamics - Stars: AGB and Post-AGB - Stars: Winds, Outflows
Simbad objects: 3
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