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

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

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..275..374c&link_type=abstract

Jets at all Scales, Proceedings of the International Astronomical Union, IAU Symposium, Volume 275, p. 374-382

Astronomy and Astrophysics

Astronomy

1

Stars: Pre-Main-Sequence, Stars: Winds, Outflows, Ism: Jets And Outflows, Ism: Molecules

Scientific paper

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.

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