Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-26T17:45:44.426Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
Sergei Plachinda
Affiliation:
Crimean Astrophysical Observatory, 298409, Nauchny, Crimea email: [email protected]
Dilyara Baklanova
Affiliation:
Crimean Astrophysical Observatory, 298409, Nauchny, Crimea email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Butkovskaya, V. V. & Plachinda, S. I., 2007, A&A, 469, 1069Google Scholar
Butkovskaya, V. V., Plachinda, S. I., Bondar’, N. I., & Baklanova, D. N., 2017, Astronomische Nachrichten, 338, 896Google Scholar
Butkovskaya, V. V., Plachinda, S. I., Baklanova, D., & Pankov, N. F., 2018, Contributions of the Astronomical Observatory Skalnaté Pleso, 48, 273Google Scholar
Chugainov, P. F. 1966, IBVS, 122Google Scholar
Plachinda, S. 2004, in: Stepanov, A. V., Benevolenskaya, E. E. & Kosovichev, A. G. (eds.), Multi-Wavelength Investigations of Solar Activity (Proceedings IAU Symposium No. 223), p. 689Google Scholar
Plachinda, S., Pankov, N., & Baklanova, D., 2011, Astronomische Nachrichten, 332, 918Google Scholar
Plachinda, S. I., Baklanova, D. N., Butkovskaya, V. V., & Pankov, N. F. 2017, in Yu. Balega, Yu., Kudryavtsev, D. O., Romanyuk, I. I., & Yakunin, I. A. (eds.), Stars: From Collapse to Collapse, (San Francisco: Astronomical Society of the Pacific), p. 247Google Scholar
Boro Saikia, S., Jeffers, S. V., Morin, J., et al. 2016, A&A, 594, id.A29Google Scholar
Severny, A., 1969, Nature, 224, 53Google Scholar