Magnetic Field Structures of Chemically Peculiar Stars. II. HD98088, HD182180, HD221218, HD318107

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

Astrophysics Pub Date : 2024-05-17 DOI:10.1007/s10511-024-09814-5

Yu. V. Glagolevskij

引用次数: 0

Abstract

Based on published data on the magnitudes of the magnetic field, models are constructed of several magnetic stars of different types of peculiarity and the parameters of the magnetic field are obtained. Among the hot objects, differences are also discovered in the physical conditions in the regions of the magnetic equators and in the region near the magnetic poles, which are not yet amenable to interpretation.

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化学奇特恒星的磁场结构。II.HD98088、HD182180、HD221218、HD318107

根据已公布的磁场大小数据，构建了几颗不同类型的磁星模型，并获得了磁场参数。在热天体中，还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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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.