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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
Abstract
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
- Information
- Proceedings of the International Astronomical Union , Volume 6 , Symposium S275: Jets at all Scales , September 2010 , pp. 374 - 382
- Copyright
- Copyright © International Astronomical Union 2011
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