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

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

Abstract

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.

Keywords

Accretion Disk Stellar Wind Magnetic Surface Young Star Tauri Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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© Springer-Verlag Berlin Heidelberg 2009

Authors and Affiliations

  1. 1.Laboratoire d’Astrophysique de GrenobleGrenobleFrance

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