大质量恒星和超新星的演化

IF 0.7 4区物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS

Astronomy Reports Pub Date : 2025-02-26 DOI:10.1134/S1063772924701154

G. S. Bisnovatyi-Kogan

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引用次数: 0

摘要

本文回顾了恒星演化的各个阶段以及演化的最后阶段。考虑了大质量恒星的核演化，不同质量恒星的动态稳定性和临界状态，超新星爆炸及其机制，特别是磁旋转模型。讨论了宇宙伽玛射线暴与超新星之间的联系。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Evolution of Massive Stars and Supernovae

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Evolution of Massive Stars and Supernovae

The paper reviews the various stages of stellar evolution and the final stages of this evolution. The nuclear evolution of massive stars, the dynamic stability and critical states of stars of various masses, supernova explosions and their mechanisms, particularly the magneto-rotational model, are considered. The connection between cosmic gamma-ray bursts and supernovae is discussed.

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来源期刊

Astronomy Reports 地学天文-天文与天体物理

CiteScore

1.40

自引率

20.00%

发文量

审稿时长

6-12 weeks

期刊介绍： Astronomy Reports is an international peer reviewed journal that publishes original papers on astronomical topics, including theoretical and observational astrophysics, physics of the Sun, planetary astrophysics, radio astronomy, stellar astronomy, celestial mechanics, and astronomy methods and instrumentation.