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Magnetic Field of Late-Type Stars: A New Approach∗

Published online by Cambridge University Press:  19 July 2016

G. Mathys  and
S. K. Solanki
G. Mathys
Affiliation:
Geneva Observatory, ch. des Maillettes 51, CH-1290 Sauverny, Switzerland
S. K. Solanki
Affiliation:
Institute of Astronomy, ETH–Zentrum, CH–8092 Zurich, Switzerland

Abstract

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Magnetic field diagnosis in three late-type stars is performed using the multiline technique originally developed by Stenflo and Lindegren (1977) to study spatially unresolved magnetic features on the sun.

Type
V. Magnetic Pieuds
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 325 - 328
Copyright
Copyright © Kluwer 1988 

References

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