Astrometry and high-speed photometry of an optical candidate for PSR 1913 + 16

Details Astrometry and high-speed photometry of an optical candidate for PSR 1913 + 16 Astrometry and high-speed photometry of an optical candidate for PSR 1913 + 16

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192p..51e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 51P-58P.

Astronomy and Astrophysics

Astronomy

2

Astrometry, Binary Stars, Pulsars, Stellar Spectrophotometry, Orbits, Photographic Plates, Star Distribution, Stellar Rotation, Tables (Data)

Scientific paper

A deep IIIaF plate has been obtained at the prime focus of the AAT which shows the candidate star described by Kristian and Westphal (1978) and Crane et al. (1979) near the timing position of the binary pulsar PSR 1913 + 16. The astrometry carried out shows that this star does not coincide with the timing position. High-speed photometry of the candidate shows no evidence for pulsations down to a time-averaged R magnitude of 26.5.

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