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Magnetic Stars in Clusters of Different Ages. II. Open Clusters IC 4756, \(\boldsymbol{\alpha}\) Per and NGC 7092

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Abstract

This paper presents the results of magnetic field measurements for 19 chemically peculiar stars in three open star clusters IC 4756, \(\alpha\) Per, NGC 7092. More than 80 spectra of circularly polarized radiation were obtained with the Main Stellar Spectrograph (MSS) at the 6-m BTA telescope of SAO RAS. It was found that the magnetic field value in these clusters is more than three times less than in the young Orion OB1 association. Apparently, unique conditions developed in this association allowed the generation of super-strong magnetic field during the formation of stars.

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Notes

  1. https://webda.physics.muni.cz/.

  2. https://www.sao.ru/hq/lizm/mss/en/index.html.

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ACKNOWLEDGMENTS

The work used the SIMBAD, VizieR, WEBDA databases and the NASA’s Astrophysics Data System (ADS). Observations with the SAO RAS telescopes are supported by the Ministry of Science and Higher Education of the Russian Federation. The renovation of telescope equipment is currently provided within the national project ’’Science and universities’’.

Funding

Observations, processing of the spectroscopic material, magnetic measurements, and analysis of the physical parameters were carried out thanks to funding from the Russian Science Foundation (grant No. 21-12-00147).

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Authors and Affiliations

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

    I. I. Romanyuk, A. V. Moiseeva, I. A. Yakunin & V. N. Aitov

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  1. I. I. Romanyuk
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  2. A. V. Moiseeva
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  3. I. A. Yakunin
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Translated by E. Porfiryeva

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Romanyuk, I.I., Moiseeva, A.V., Yakunin, I.A. et al. Magnetic Stars in Clusters of Different Ages. II. Open Clusters IC 4756, \(\boldsymbol{\alpha}\) Per and NGC 7092. Astrophys. Bull. 78, 152–164 (2023). https://doi.org/10.1134/S1990341323020062

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