Modeling Accretion and Ejection Phenomena Around Young Stars: A Numerical Perspective

  • Claudio ZanniEmail author
Part of the Lecture Notes in Physics book series (LNP, volume 791)


This chapter presents an overview of models based on time-dependent numerical simulations of the central regions of accreting T Tauri stars. The focus is put on magnetohydrodynamical studies of the launching mechanism of T Tauri jets (disk–winds, stellar winds, magnetospheric ejections) and of the magnetic star–disk interaction.


Accretion Disk Stellar Wind Magnetic Surface Young Star Tauri Star 
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© Springer-Verlag Berlin Heidelberg 2009

Authors and Affiliations

  1. 1.Laboratoire d’Astrophysique de GrenobleGrenobleFrance

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