Email this article On Properties of Main Sequence Magnetic Stars
- Authors: Glagolevskij Y.V.1
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Affiliations:
- Special Astrophysical Observatory
- Issue: Vol 74, No 1 (2019)
- Pages: 66-79
- Section: Article
- URL: https://journal-vniispk.ru/1990-3413/article/view/212851
- DOI: https://doi.org/10.1134/S1990341319010073
- ID: 212851
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Abstract
We reconsidered the previous studies of properties of magnetic stars based on the latest data on average surface magnetic fields of 177 stars. New, corrected results have been obtained that allow a better understanding of the phenomenon of magnetic chemically peculiar stars.
About the authors
Yu. V. Glagolevskij
Special Astrophysical Observatory
Author for correspondence.
Email: glagol@sao.ru
Russian Federation, Nizhnii Arkhyz, 369167
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