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Spectropolarimetric study of selected cool supergiants

Published online by Cambridge University Press:  23 January 2015

V. Butkovskaya ,
S. Plachinda  and
D. Baklanova
V. Butkovskaya
Affiliation:
Crimean Astrophysical Observatory of Taras Shevchenko National University of Kyiv, 98409, Nauchny, Crimea, Ukraine email: [email protected]
S. Plachinda
Affiliation:
Crimean Astrophysical Observatory of Taras Shevchenko National University of Kyiv, 98409, Nauchny, Crimea, Ukraine email: [email protected]
D. Baklanova
Affiliation:
Crimean Astrophysical Observatory of Taras Shevchenko National University of Kyiv, 98409, Nauchny, Crimea, Ukraine email: [email protected]
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Abstract

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Cool supergiants offer a good opportunity to study the interplay of magnetic fields and stellar evolution. We present the results of spectropolarimetric study of the cool supergiants and classical Cepheids η Aql and ζ Gem.

Keywords

Stars: magnetic fieldssupergiantsCepheidsstars: individual (η Aql, ζ Gem)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 369 - 370
Copyright
Copyright © International Astronomical Union 2015 

References

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