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Direct detection of a magnetic field on the surface of slowly rotating giant stars

Published online by Cambridge University Press:  01 November 2008

Michel Aurière ,
R. Konstantinova-Antova ,
P. Petit ,
G. Wade  and
T. Roudier
Michel Aurière
Affiliation:
LATT, CNRS, University of Toulouse, 57 Avenue d'Azereix, 65008 Tarbes, France, email: name@ast.obs-mip.fr
R. Konstantinova-Antova
Affiliation:
Institute of Astronomy, BAS, 72 Tsarigradsko shose, 1784 Sofia, Bulgaria, email: renada@astro.bas.bg
P. Petit
Affiliation:
LATT, CNRS, University of Toulouse, 57 Avenue d'Azereix, 65008 Tarbes, France, email: name@ast.obs-mip.fr
G. Wade
Affiliation:
Department of Physics, RMC, PO Box 17000, Station “Forces”, Kingston, K7K4B4 Ontario, Canada email: gregg.wade@rmc.ca
T. Roudier
Affiliation:
LATT, CNRS, University of Toulouse, 57 Avenue d'Azereix, 65008 Tarbes, France, email: name@ast.obs-mip.fr
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Abstract

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We present first results of the magnetic survey of a sample of slow rotating giant stars for which an X-ray emission or variations of CaII H & K lines have been already detected.

Keywords

Stars: late type – stars: magnetic fields
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S259: Cosmic Magnetic Fields: From Planets, to Stars and Galaxies , November 2008 , pp. 431 - 432
Copyright
Copyright © International Astronomical Union 2009

References

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