Binary and Millisecond Pulsars

被引：9
作者：
Lorimer D.R. [1 ]
机构：
[1] Max Planck Institut für Radioastronomie, Auf dem Hügel 69, Bonn
来源：
Living Reviews in Relativity | 1998年 / 1卷 / 1期
关键词：
Millisecond Pulsars; Neutron Star; post-Keplerian Parameters; Gravity Wave Detectors; Local Surface Density;
D O I：
10.12942/lrr-1998-10
中图分类号：
学科分类号：
摘要：
Our knowledge of binary and millisecond pulsars has greatly increased in recent years. This is largely due to the success of large-area surveys which have brought the known population of such systems in the Galactic disk to around 50. As well as being interesting as a population of astronomical sources, many pulsars turn out to be superb celestial clocks. In this review we summarise the main properties of binary and millisecond pulsars and highlight some of their applications to relativistic astrophysics. © 1998, The Author(s).
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