无线电波霎

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/S1063772924701130

G. S. Bisnovatyi-Kogan

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引用次数: 0

摘要

本文综述了射电脉冲星的理论和观测。介绍了倾斜旋转体模型、单极发生器：Goldreich-Julian模型、旋转能量损失、制动指数、星震和周期跳跃、脉冲星、双星和循环射电脉冲星的磁场、中子星质量的测定、中子星合并过程中引力波的发射、宇宙伽马射线暴。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

Radio Pulsars

查看原文本刊更多论文

Radio Pulsars

The paper is a review of the theory and observations of radio pulsars. The inclined rotator model, unipolar generator: Goldreich–Julian model, rotational energy losses, braking index, starquakes and period jumps, magnetic fields of pulsars, binary and recycled radio pulsars, determination of neutron star masses, emission of gravitational waves during the merger of neutron stars, cosmic gamma-ray bursts are described.

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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.