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À propos de : Observing and Modelling Stellar Magnetic Fields        

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  • 3. Structure and Evolution
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  • Observing and Modelling Stellar Magnetic Fields
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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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  • eas0939003
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  • © EAS, EDP Sciences, 2009
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  • EAS, EDP Sciences
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