Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-30T23:05:33.674Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsar as barycenter coordinate clock

Published online by Cambridge University Press:  01 August 2006

Yuri P. Ilyasov ,
S. M. Kopeikin ,
Mikhail V. Sazhin  and
Vladimir E. Zharov
Yuri P. Ilyasov
Affiliation:
Pushchino Radio Astronomical Observatory, Lebedev Physical Institute, Leninskii prosp 53, RU-142290 Puschino, Russian Federation email: [email protected]
S. M. Kopeikin
Affiliation:
Department of Physics and Astronomy, University of Missouri, 322 Physics Building, Columbia, MO 65211, USA
Mikhail V. Sazhin
Affiliation:
Sternberg Astronomical Institut, Moscow State University, Universitetskij pr., 13, RU-119992 Moscow, Russian Federation email: [email protected], [email protected]
Vladimir E. Zharov
Affiliation:
Sternberg Astronomical Institut, Moscow State University, Universitetskij pr., 13, RU-119992 Moscow, Russian Federation email: [email protected], [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Pulsars can be considered as very precise clocks if they are observed from the barycenter of the Solar system. Pulsar Timing Array (PTA) can be used to establish new astronomical reference frame which describes both space and time properties. Among these arrays most remarkable are the Parks Pulsar Timing Array (PPTA) and Kalyazin Pulsar Timing Array (KPTA).

Keywords

pulsars: generaltimestandards
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 479
Copyright
Copyright © International Astronomical Union 2007