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Spectropolarimetric study of selected cool supergiants

Published online by Cambridge University Press:  23 January 2015

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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Auriere, M. e. a. 2010, A&A 516, L2Google Scholar
Butkovskaya, V. 2014a, in Magnetic fields throughout stellar evolution, Vol. 302 of IAU Symposium, in pressGoogle Scholar
Butkovskaya, V. 2014b, in Precision Asteroseismology, Vol. 301 of IAU Symposium, pp 393–394CrossRefGoogle Scholar
Butkovskaya, V. & Plachinda, S. 2007, A&A 469, 1069Google Scholar
Grunhut, J. E. A. 2010, MNRAS 408, 2290Google Scholar
Plachinda, S. 2000, A&A 360, 642Google Scholar
Plachinda, S. 2005, Astrophysics 48, 9CrossRefGoogle Scholar