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Magnetic CP stars in Orion OB1 association

Published online by Cambridge University Press:  23 January 2015

Iosif I. Romanyuk  and
Eugene A. Semenko
Iosif I. Romanyuk
Affiliation:
Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnii Arkhyz, Russian Federation, 369167 email: roman@sao.ru, sea@sao.ru
Eugene A. Semenko
Affiliation:
Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnii Arkhyz, Russian Federation, 369167 email: roman@sao.ru, sea@sao.ru
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Abstract

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We present the overview of an observational program carring out on the 6-m telescope of Special Astrophysical Observatory from 2012. This program aims the searches of new Bp stars with surface magnetic field and the detailed study of known magnetic CP star from the stellar association Ori OB1. HD 34736 is the most interesting star that was found as magnetic within the program recently.

Keywords

stars: evolutionopen clusters and associations: generalstars: magnetic fieldsstars: chemically peculiar
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. 393 - 394
Copyright
Copyright © International Astronomical Union 2015 

References

Romanyuk, I. I., Semenko, E. A., Yakunin, I. A., & Kudryavtsev, D. O. 2013, Astrophysical Bulletin 68, 300Google Scholar
Semenko, E. A., Romanyuk, I. I., Kudryavtsev, D. O., & Yakunin, I. A. 2014, Astrophysical Bulletin 69, 191Google Scholar