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Observing and Modelling StellarMagnetic Fields

3. Structure and Evolution

Published online by Cambridge University Press:  03 November 2009

C. Neiner ,
J.-P. Zahn  and
J.D. Landstreet
J.D. Landstreet*
Affiliation:
Dept. of Physics & Astronomy, University of Western Ontario, London, ON N6A 3K7, Canada
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Abstract

We start by looking at some recent developments in field measurements in middle main sequence and pre-main sequence stars. Then we consider how other magnetic effects such as the Hanle effect and continuum polarisation may be used to detect fields in a variety of stellar environments such as the solar corona and white dwarf atmospheres. Finally we consider how the current body of observational knowledge about magnetic stars may be integrated into a roughly coherent, provisional scenario of field origin and evolution.

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Type
Research Article
Information
European Astronomical Society Publications Series , Volume 39: Stellar Magnetism , 2009 , pp. 39 - 53
Copyright
© EAS, EDP Sciences, 2009

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