Hostname: page-component-5c6d5d7d68-wtssw Total loading time: 0 Render date: 2024-08-07T09:22:59.014Z Has data issue: false hasContentIssue false

On Bipolar Jet Formation in Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

G. Pascoli*
Affiliation:
Faculté des Sciences, Department of Physics, Amiens, France

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Bipolar outflows or polar knots are rather ubiquitous phenomena. A wealth of observational data is now available on bipolar flows associated with young stellar objects or stellar formation regions (Snell, Proc. I. A. U. Symp. Nr. 115, 1987), or nuclei of active galaxies (Asseo and Sol, 1987, Phys. Rep. 148, 307).

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Copyright
Copyright © Kluwer 1993