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Long-term stellar magnetic field study at the Crimean Astrophysical Observatory

Published online by Cambridge University Press:  27 November 2018

Varvara Butkovskaya Open the ORCID record for Varvara Butkovskaya [Opens in a new window] ,
Sergei Plachinda  and
Dilyara Baklanova
Varvara Butkovskaya
Affiliation:
Crimean Astrophysical Observatory, 298409, Nauchny, Crimea email: vb@craocrimea.ru
Sergei Plachinda
Affiliation:
Crimean Astrophysical Observatory, 298409, Nauchny, Crimea email: vb@craocrimea.ru
Dilyara Baklanova
Affiliation:
Crimean Astrophysical Observatory, 298409, Nauchny, Crimea email: vb@craocrimea.ru
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Abstract

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The long-term monitoring of magnetic cycles is a key diagnostic in understanding how dynamo generation and amplification of magnetic fields occur in solar-like stars. One of the current key problems is the establishment of the magnetic field behavior during the activity cycles for stars of different ages and evolutionary statuses. We present the experience of using own long-term datasets for study of activity cycles in selected stars at the Crimean Astrophysical Observatory.

Keywords

Techniques: spectropolarimetricstars: atmospheresstars: activitystars: magnetic fieldsstars: late-typestars: oscillations
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 35 - 38
Copyright
Copyright © International Astronomical Union 2018 

References

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