Neutron stars - How pulsars get their spins

被引：2

作者：

Burrows, A ^{[1
]}

机构：

[1] Univ Arizona, Dept Astron, Tucson, AZ 85721 USA

来源：

NATURE | 1998年 / 393卷 / 6681期

关键词：

D O I：

10.1038/30108

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

A supernova explosion announces the spectacular death of a massive star. The remnant is usually a neutron star, tiny and dense, and often spinning rapidly and travelling at high speed through the Galaxy. A provocative new thesis forms a bridge between the physics of supernovae and the spin and velocity of neutron stars.

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页码：121 / 122

页数：2

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