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A precessing jet in L1551

Published online by Cambridge University Press:  04 August 2017

J. F. Lightfoot*
Affiliation:
Department of Physics and Astronomy, University College London, Gower Street London WC1E 6BT

Abstract

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An analysis of published observations of the L1551 optical jet leads to the conclusion that the driving region is very small, possibly little larger than the star itself. Further the data suggest that the jet is precessing.

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

References

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