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New results form HST on fast, colimated outflows in dying stars - the primary mechanism for shaping planetary nebulaeIn this paper, we briefly describe the results from imaging surveys of young PNe and PPNe with HST, and then present new results from detailed kinematic studies of several prominent objects which support our hypothesis for shaping PNe.
Document ID
20060030565
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
External Source(s)
hdl:2014/11249
Authors
Sahai, R.
Contreras, C.
Date Acquired
August 23, 2013
Publication Date
January 5, 2003
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Other
Keywords
HST outflows planetary nebulae

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