Abstract (EN):
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.
Idioma:
Inglês
Tipo (Avaliação Docente):
Científica
Nº de páginas:
4