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The RW Aur microjet: testing MHD disk wind models
Authors:C Dougados  S Cabrit  L Lopez-Martin  P Garcia  D O'Brien
Institution:1. Laboratoire d'Astrophysique de l'Observatoire de Grenoble, USA E-mail
2. Observatoire de Paris, LERMA –, USA
3. University of Porto, Portugal
Abstract:We conduct a detailed comparison between the kinematics, morpology and excitation conditions of the RW Aur microjet on scales < 200 AU with predictions from stationary, self-similar, cold disk wind solutions. Implications for launching and ionization mechanisms of jets in young stars are discussed.
Keywords:
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