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Statistical Properties of Magnetic CP Stars

Published online by Cambridge University Press:  26 May 2016

S. Bagnulo
S. Bagnulo*
Affiliation:
European Southern Observatory, Alonso de Cordova 3107, Santiago, Chile

Abstract

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Magnetic fields of chemically peculiar (CP) stars of the upper main sequence are characterised by a geometry organised at a large scale, permeating the entire photosphere, and with a typical strength of the order of 0.1–30 kG. Here I review the results obtained from statistical studies of the structures of the magnetic fields of CP stars, which are aimed at finding how magnetic strength and morphology are correlated with other stellar characteristics and with the star's evolutionary state.

Type
Session D. Atmospheric Inhomogeneities
Information
Symposium - International Astronomical Union , Volume 210: Modelling of Stellar Atmospheres , 2003 , pp. 209 - 220
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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