大质量 O 型星 HD 37022、HD 191612 和 HD 149438 的磁场结构

IF 1.3 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Astrophysical Bulletin Pub Date : 2024-07-31 DOI:10.1134/S1990341324600595

Yu. V. Glagolevskij

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引用次数: 0

摘要

摘要对磁性O星和强氦天体的性质进行比较后发现，它们之间存在着家族联系；它们的形成和进一步演化的机制显然是相同的。磁性O星家族延续了已知磁性Ap天体的序列，向更高的质量演化。观测到的性质差异与O天体的大质量有关。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Structure of the Magnetic Field of Massive O Stars HD 37022, HD 191612, HD 149438

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Structure of the Magnetic Field of Massive O Stars HD 37022, HD 191612, HD 149438

Comparison of the properties of magnetic O stars with He-strong objects showed their family connection; the mechanism of their formation and further evolution is obviously the same. The family of magnetic O stars continues the sequence of known magnetic Ap objects towards higher masses. The observed differences in properties are associated with the large mass of O objects.

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来源期刊

Astrophysical Bulletin 地学天文-天文与天体物理

CiteScore

2.00

自引率

33.30%

发文量

审稿时长

>12 weeks

期刊介绍： Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.