Literature DB >> 28937181

Binary and Millisecond Pulsars.

D R Lorimer1.   

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


  4 in total

1.  Pulsar timing limits on very low frequency stochastic gravitational radiation.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1996-03-15

2.  Cosmological constraints on cosmic-string gravitational radiation.

Authors: 
Journal:  Phys Rev D Part Fields       Date:  1992-05-15

3.  Cosmic gravitational-wave background: Limits from millisecond pulsar timing.

Authors: 
Journal:  Phys Rev Lett       Date:  1990-07-16       Impact factor: 9.161

4.  Confirmation of Earth-Mass Planets Orbiting the Millisecond Pulsar PSR B1257 + 12.

Authors:  A Wolszczan
Journal:  Science       Date:  1994-04-22       Impact factor: 47.728

  4 in total
  1 in total

Review 1.  The Confrontation between General Relativity and Experiment.

Authors:  Clifford M Will
Journal:  Living Rev Relativ       Date:  2001-05-11       Impact factor: 40.429

  1 in total

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