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New Infrared Measurements of Magnetic Fields on Cool Stars

Published online by Cambridge University Press:  03 August 2017

Steven H. Saar*
Affiliation:
Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, U.S.A.

Abstract

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I present a preliminary analysis of IR spectra of five K and M dwarfs and two RS CVn variables. Evidence for significant magnetic flux is found on several stars, a number of which are detected for the first time. Field strengths (B) on the RS CVn variables are lower than in the active dwarfs, consistent with the concept of pressure balance limiting B in stellar photospheres. I compare the results with previous measurements.

Type
Part 5: Magnetic Fields and Infrared Magnetometry
Copyright
Copyright © Kluwer 1994 

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