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Results of magnetic field measurements of CP stars carried out with the Russian 6-m telescope. I. Observations in 2007

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Abstract

This paper presents the results of magnetic field measurements for 39 chemically peculiar and 3 normal main sequence stars used as standard stars. Observations were carried out with the Main Stellar Spectrograph of the Russian 6-m telescope during 2007. Zeeman measurements for 8 stars were performed for the first time. The accuracy analysis for the longitudinal magnetic field measurements of the stars confirms that the systematic errors do not exceed 10–20 G and are within the quoted limits. The absence of significant instrumental deviations follows from the measurements of the CP stars with well-known B e variation curves.

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Authors and Affiliations

  1. Special Astrophysical Observatory, Russian Academy of Sciences, Nizhnii Arkhyz, 369167, Russia

    I. I. Romanyuk, E. A. Semenko & D. O. Kudryavtsev

Authors
  1. I. I. Romanyuk
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  2. E. A. Semenko
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  3. D. O. Kudryavtsev
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Correspondence to I. I. Romanyuk.

Additional information

Original Russian Text © I.I. Romanyuk, E.A. Semenko, D.O. Kudryavtsev, 2014, published in Astrofizicheskii Byulleten, 2014, Vol. 69, No. 4, pp. 451–463.

The paper is based on the analysis of the spectral data obtained with the 6-m telescope BTA of the Special Astrophysical Observatory.

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Romanyuk, I.I., Semenko, E.A. & Kudryavtsev, D.O. Results of magnetic field measurements of CP stars carried out with the Russian 6-m telescope. I. Observations in 2007. Astrophys. Bull. 69, 427–438 (2014). https://doi.org/10.1134/S1990341314040051

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  • DOI: https://doi.org/10.1134/S1990341314040051

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