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Magnetic Accretion Model for the Activities of Very Young Stars
Published online by Cambridge University Press: 12 April 2016
Abstract:
A magnetodynamic model is proposed to interpret the observed inflow-outflow-X-ray emitting region complex in the atmospheres of T Tau stars.
- Type
- Session IV: Theoretical Aspects
- Information
- International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 625 - 627
- Copyright
- Copyright © Reidel 1983
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