A new determination of the position of the VELA pulsar

Details A new determination of the position of the VELA pulsar A new determination of the position of the VELA pulsar

May 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.179p..51g&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 179, May 1977, p. 51P-54P.

Astronomy and Astrophysics

Astronomy

1

Astrometry, Position (Location), Pulsars, Radio Astronomy, Radio Telescopes, Stellar Luminosity, Transits

Scientific paper

Observations have been made with the Fleurs synthesis telescope at 1415 MHz and the Molonglo radio telescope at 408 MHz to determine the position of the Vela pulsar, PSR 0833-45. When combined with earlier measurements, these data give a mean position with rms errors of about 0.8 arcsec. This mean position is quite close to the optical identification suggested by Lasker (1976).

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