Astrophysical Jets with Conical Wire Arrays: Radiative Cooling, Rotation & Deflection

Details Astrophysical Jets with Conical Wire Arrays: Radiative Cooling, Rotation & Deflection Astrophysical Jets with Conical Wire Arrays: Radiative Cooling, Rotation & Deflection

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1088...83a&link_type=abstract

DENSE Z-PINCHES: Proceedings of the 7th International Conference on Dense Z-Pinches. AIP Conference Proceedings, Volume 1088, p

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Z-Pinches, Plasma Focus, And Other Pinch Devices, Supersonic And Hypersonic Flows, Plasma Diagnostic Techniques And Instrumentation

Scientific paper

Highly collimated outflows or jets are produced by a number of astrophysical objects including protostars. The morphology and collimation of these jets is thought to be strongly influenced by the effects of radiative cooling, angular momentum and the interstellar medium surrounding the jet. Astrophysically relevant experiments are performed with conical wire array z-pinches investigating each of these effects. It is possible in each case to enter the appropriate parameter regime, leading the way towards future experiments where these different techniques can be more fully combined.

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