脉冲星、中子星与夸克星

自然杂志 ›› 2007, Vol. 29 ›› Issue (4): 200-203.

脉冲星、中子星与夸克星

②徐峰① 岳友岭② 徐仁新③

①②博士，③教授，博士生导师北京大学物理学院，北京100871

收稿日期:2007-04-10 修回日期:2007-05-10 出版日期:2007-08-20 发布日期:2007-08-20

Pulsar, Neutron Star, and Quark Star

XU Feng① YUE You-ling① XU Ren-xin③

①②Ph.D.，③professor Department of Astronomy, School of Physics, Peking University, Beijing 100871

Received:2007-04-10 Revised:2007-05-10 Online:2007-08-20 Published:2007-08-20

摘要/Abstract

摘要： 关于观测到脉冲星的本质目前存有两种看法：中子星和夸克星。本文简述了相关的研究历史以及这些天体的基本性质和可能观测表现。展望了我国在此研究方向的发展前景。

关键词: 脉冲星, 中子星, 夸克星

Abstract: Neutron stars and quark stars are currently two kinds of speculated bodies when one is modeling observed pulsars. After a brief introduction to the related history, the characters and possible observational features of these objects are focused on. A future perspective on the pulsar research in China is presented.

Key words: pulsars, neutron stars, quark stars

徐峰;岳友岭;徐仁新. 脉冲星、中子星与夸克星[J]. 自然杂志, 2007, 29(4): 200-203.

XU Feng;YUE You-ling;XU Ren-xin. Pulsar, Neutron Star, and Quark Star[J]. Chinese Journal of Nature, 2007, 29(4): 200-203.