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Molecular and atomic jets in young low-mass stars: Properties and origin

Published online by Cambridge University Press:  24 February 2011

Sylvie Cabrit
Affiliation:
LERMA, Observatoire de Paris, CNRS 61 Avenue de l'Observatoire, F-75014Paris email: [email protected]
J. Ferreira
Affiliation:
LAOG, Observatoire de Grenoble, CNRS email: [email protected], [email protected]
C. Dougados
Affiliation:
LAOG, Observatoire de Grenoble, CNRS email: [email protected], [email protected]
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Abstract

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The key characteristics of molecular and atomic ejection from young stars are summarized, with emphasis on similarities across evolutionary stages, and the need for efficient magnetic collimation and ejection extracting a large fraction of the accretion power. The jet kinematics, and its dust and molecular content, are confronted to steady MHD jet models, and the probable contribution of non-steady processes is pointed out.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2011

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