Hostname: page-component-cd9895bd7-fscjk Total loading time: 0 Render date: 2024-12-27T11:06:09.097Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic fields in the photospheres of main sequence A and B stars: Observations, models, theories and mysteries

Published online by Cambridge University Press:  17 November 2003

J. Arnaud ,
N. Meunier  and
J. D. Landstreet
J. D. Landstreet*
Affiliation:
Department of Physics & Astronomy, University of Western Ontario, London, Ontario, Canada
Get access

Abstract

This review presents a general overview of the magnetic fields foundin main sequence A and B stars, and of some of the phenomenaassociated with this magnetism. An attempt is made to place theobserved magnetic fields into an evolutionary context.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 9: Magnetism and Activity of the Sun and Stars , 2003 , pp. 235
Copyright
© EAS, EDP Sciences, 2003

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)