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Chromospheric activity of 9 Aurigae

Published online by Cambridge University Press:  18 February 2014

Anthony B. Kaye ,
Cristine Kristof  and
Richard O. Gray
Anthony B. Kaye
Affiliation:
Department of Physics, Texas Tech University Lubbock, Texas 79409-1051, United States of America email:anthony.kaye@ttu.edu
Cristine Kristof
Affiliation:
Department of Physics, Texas Tech University Lubbock, Texas 79409-1051, United States of America email:anthony.kaye@ttu.edu
Richard O. Gray
Affiliation:
Department of Physics and Astronomy, Appalachian State University Boone, North Carolina 28608, United States of America email:grayro@appstate.edu
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Abstract

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The definition of γ Dor stars as a new class of variable stars by Kaye et al. (1999) was based on a number of criteria, including the failure to detect any emission in the Ca II H & K lines in these stars (Kaye & Strassmeier 1998; KS98). Over the last 30 years, efforts continue to look for the blue edge of chromospheric activity. As a part of this effort, we put γ Dor stars to the test to see if magnetic fields play a non-trivial role in their variability.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 439 - 440
Copyright
Copyright © International Astronomical Union 2014 

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