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Hypersonic jets from young stars in molecular clouds

Published online by Cambridge University Press:  04 August 2017

Hans-Joachim Blome
Affiliation:
Inst. f. Theoretische Physik (SFB 301), D-5 Köln 41
Wolfgang Kundt
Affiliation:
Inst. f. Astrophysik, D-53 Bonn 1

Abstract

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We argue that the narrow jets which are sometimes seen to escape from YSOs into an ambient molecular cloud consist of e±-plasma which can be created in stellar magnetospheric discharges and subsequently centrifugally post-accelerated. This high-pressure pair plasma is squeezed into two jets which ram cocoons into the molecular cloud, observed in the form of molecular lobes (outflows).

Type
Bipolar Flows, Jets and Protostars
Copyright
Copyright © Reidel 1987 

References

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