高质量恒星的磁性

IF 3.2 Q2 ASTRONOMY & ASTROPHYSICS Galaxies Pub Date : 2023-03-05 DOI:10.3390/galaxies11020040

Z. Keszthelyi

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引用次数: 1

摘要

磁性是天体物理等离子体中普遍存在的特性，但恒星的磁性仍远未被完全理解。在这篇综述中，我们描述了最近的观测和建模工作，以及扩大我们对高质量恒星磁特性知识的进展。几种机制（磁对流、质量损失猝灭、内部角动量输运和磁制动）对恒星演化、种群和最终产物具有重要意义。因此，解决和解决与高质量恒星磁性相关的悬而未决的问题仍然是一个紧迫的问题。

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Magnetism in High-Mass Stars

Magnetism is a ubiquitous property of astrophysical plasmas, yet stellar magnetism still remains far from being completely understood. In this review, we describe recent observational and modelling efforts and progress to expand our knowledge of the magnetic properties of high-mass stars. Several mechanisms (magneto-convection, mass-loss quenching, internal angular momentum transport, and magnetic braking) have significant implications for stellar evolution, populations, and end-products. Consequently, it remains an urgent issue to address and resolve open questions related to magnetism in high-mass stars.

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来源期刊

Galaxies Physics and Astronomy-Astronomy and Astrophysics

CiteScore

4.90

自引率

12.00%

发文量

100

审稿时长

11 weeks

期刊介绍： Es una revista internacional de acceso abierto revisada por pares que proporciona un foro avanzado para estudios relacionados con astronomía, astrofísica y cosmología. Areas temáticas Astronomía Astrofísica Cosmología Astronomía observacional: radio, infrarrojo, óptico, rayos X, neutrino, etc. Ciencia planetaria Equipos y tecnologías de astronomía. Ingeniería Aeroespacial Análisis de datos astronómicos. Astroquímica y Astrobiología. Arqueoastronomía Historia de la astronomía y cosmología. Problemas filosóficos en cosmología.