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Pulsar Astrometry—Availabilities and Relativistic Aspects of a Pulsar Reference Frame

Published online by Cambridge University Press:  19 July 2016

O.V. Doroshenko ,
Yu.P. Ilyasov ,
S.M. Kopejkin  and
M.V. Sazhin
O.V. Doroshenko
Affiliation:
Lebedev Physical Institute Leninskii pros. 53 117924 Moscow, USSR
Yu.P. Ilyasov
Affiliation:
Lebedev Physical Institute Leninskii pros. 53 117924 Moscow, USSR
S.M. Kopejkin
Affiliation:
Sternberg State Astronomical Institute Universitetskii pros. 13 119899 Moscow, USSR
M.V. Sazhin
Affiliation:
Sternberg State Astronomical Institute Universitetskii pros. 13 119899 Moscow, USSR

Abstract

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We propose a quasi-inertial four-dimensional reference frame in the solar system asymptotically-flat spacetime on the basis of pulsar astrometry techniques. The Pulsar Reference Frame (PRF) consists of the Pulsar Time Scale (PT) and the the Pulsar Reference System (PRS) on the sky.

Type
Part 3: Concepts, Definitions, Models
Information
Symposium - International Astronomical Union , Volume 141: Inertial Coordinate System on the Sky , 1990 , pp. 213 - 216
Copyright
Copyright © Kluwer 1990 

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