University > ZAH > ITA > Institute > Colloquim >
Monday, December 5, 2011 - 11:00am
"Mechanisms for magnetically launching an outflow from a disc"
Abstract. It is now generally accepted that magnetic fields are required for launching and collimating outflows from astrophysical objects. Although several different mechanisms are proposed in the literature, the magneto-centrifugal wind model is arguably the best-known. In this talk, I will briefly review the magneto-centrifugal and magnetic tower models for outflows, and then discuss numerical simulations demonstrating that these two models are closely related.
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