化学奇特恒星的磁场结构。II.HD 98088, HD182180, HD221218, HD318107

IF 0.6 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Astrophysics Pub Date : 2024-04-08 DOI:10.54503/0002-3051-2024.77.1-41

Ю. В. Глаголевский

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引用次数: 0

摘要

根据有关磁场值的文献数据，构建了几颗不同类型的磁性恒星的磁场模型，并获得了磁场参数。在热天体中，发现了磁赤道区域和近磁极区域的物理条件差异，这些差异尚无法解释。根据有关磁场值的文献数据，构建了几颗不同类型的磁性恒星的磁场模型，并获得了磁场参数。在热天体中，发现磁赤道区域和磁极附近区域的物理条件存在差异，这些差异尚无法解释。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Структуры магнитного поля химически пекулярных звезд. II.HD 98088, HD182180, HD221218, HD318107

На основе литературных данных о величинах магнитного поля построены модели магнитного поля нескольких магнитных звезд разных типов пекулярности и получены параметры магнитного поля. Среди горячих объектов обнаружены различия физических условий в области магнитных экваторов и в области близмагнитных полюсов, которые пока не поддаются интерпретации.Based on literature data about the magnetic field values, models of the magnetic field of several magnetic stars of different types of peculiarity were constructed and the magnetic field parameters were obtained. Among hot objects, differences in physical conditions have been discovered in the region of the magnetic equators and in the region near the magnetic poles, which are not yet amenable to interpretation

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来源期刊

Astrophysics 地学天文-天文与天体物理

CiteScore

0.90

自引率

20.00%

发文量

审稿时长

6-12 weeks

期刊介绍： Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.