| Literature DB >> 28937181 |
Abstract
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. ELECTRONIC SUPPLEMENTARY MATERIAL: Supplementary material is available for this article at 10.12942/lrr-1998-10.Entities:
Year: 1998 PMID: 28937181 PMCID: PMC5567244 DOI: 10.12942/lrr-1998-10
Source DB: PubMed Journal: Living Rev Relativ ISSN: 1433-8351 Impact factor: 40.429