A possibility for the use of pulsar observations in astrometry

Details A possibility for the use of pulsar observations in astrometry A possibility for the use of pulsar observations in astrometry

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...40f&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Nov.-Dec. 1986, p. 40-46. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astrometry, Astronomical Coordinates, Extragalactic Radio Sources, Interferometry, Pulsars, Reference Systems

Scientific paper

The possibility of using pulsar observations to determine the location of an equatorial system of coordinates relative to a reference frame formed by vectors directed toward extragalactic radio sources is considered. The system is based on the combined use of interferometric and time-of-arrival observations. The problem is solved in the first approximation and it is concluded that the present method can be used to eliminate ambiguities which arise in astrometry.

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