Stellar Outflows with New Tools: Advanced Simulations and Laboratory Experiments

Details Stellar Outflows with New Tools: Advanced Simulations and Laboratory Experiments Stellar Outflows with New Tools: Advanced Simulations and Laboratory Experiments

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...85f&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astrophysics

H Ii Regions, Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

In this contribution we provide a brief overview of new numerical results describing the evolution of clumpy flows as well as new studies of magnetized winds/jets. In addition, we report on a new approach to studying these phenomena: direct laboratory experiments. Recent advances in the use of ``high energy density'' laboratory devices now allows researchers to produce scalable plasma flow experiments relevant to hypersonic astrophysical jets and shock-clump interactions in the context of circumstellar outflows.

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