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Observational and numerical tests of jet models in young stars

Published online by Cambridge University Press:  21 October 2010

S. Cabrit
S. Cabrit*
Affiliation:
LERMA, Observatoire de Paris et UMR 8112 du CNRS, 61 Av. de l'Observatoire, 75014 Paris. email: sylvie.cabrit@obspm.fr
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Abstract

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Jets are found in a wide range of accreting young stars, from brown dwarfs to massive protostars, but their launch region(s) and their role in angular momentum extraction are still debated. Many observational constraints exist on jet properties, including jet widths, kinematics along and across the jet, possible rotation signatures, ejection/accretion ratio, depletion and molecular counterparts. This contribution compares popular models, in particular disk winds, with these constraints and with MHD numerical simulations, highlighting a few open issues.

Keywords

accretion disksMHDstars: pre–main-sequenceISM: jets and outflows
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 748 - 749
Copyright
Copyright © International Astronomical Union 2010

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