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Theory of outflows

  • Arieh Königl
Part V: Outflows—Theory
Part of the Lecture Notes in Physics book series (LNP, volume 465)

Abstract

Following a brief review of the current observational picture of outflows from low- and intermediate-mass young stellar objects, various theoretical model ingredients are discussed, focusing on a scenario in which the outflows correspond to centrifugally driven winds from magnetized accretion disks. Among the topics considered are the wind kinematics and dynamics, the outflow thermal and ionization structure, and nonsteady ejection. Particular attention is paid to some of the outstanding questions in both theory and observations.

Keywords

Accretion Disk Flow Line Disk Surface Wind Model Stellar Surface 
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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Copyright information

© Springer-Verlag 1996

Authors and Affiliations

  • Arieh Königl
    • 1
  1. 1.Department of Astronomy & AstrophysicsThe University of ChicagoChicagoUSA

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