An improvement of the plate constant method in the determination of stellar parallaxes

Details An improvement of the plate constant method in the determination of stellar parallaxes An improvement of the plate constant method in the determination of stellar parallaxes

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987acasn..28..190z&link_type=abstract

(Acta Astronomica Sinica, vol. 28, 1987, p. 190-196) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 12, Sept. 1988, p

Astronomy and Astrophysics

Astrophysics

Mathematical Models, Reference Stars, Stellar Parallax, Astronomical Coordinates, Trigonometry

Scientific paper

This paper introduces self-dependence of reference stars in the method
of plate constants, which can be used to identify and reject reference
stars with unusually large proper motion or parallax. A specific example
(BD +70.68 deg) is worked out. The configuration of reference stars is
also discussed.

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