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Magnetic Activity and the Interaction Between the Stellar Magnetosphere and the Accretion Disk

  • A. I. Gómez De Castro
Chapter

Abstract

Analytical and numerical analysis of the interaction between the magnetosphere of the PreMain-Sequence (PMS) stars and accretion disks are converging to a robust, fundamental mechanism for jet formation. They provide a reasonably solid base-line to explain the current observations on the formation of solar-like stars. In this summary, the connection between observations and this paradigm are reviewed critically and some observational tests proposed.

Keywords

magnetic fields-stars: formation-circumstellar matter-stars: mass-loss planetary systems: protoplanetary discs ISM: jets and outflows 

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Copyright information

© Springer Science+Business Media Dordrecht 2004

Authors and Affiliations

  • A. I. Gómez De Castro
    • 1
  1. 1.Institute de Astronomía y Geodesia (CSIC-UCM) Fac. de CC MatemáticasUniversidad Complutense de MadridMadridSpain

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