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

Publishing date

Sep 1988

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988cha%26a..12..254z&link_type=abstract

Journals

Chinese Astronomy and Astrophysics, Volume 12, Issue 3, p. 254-259.

Science

Astronomy and Astrophysics

Field

Astrophysics

Type

Scientific paper

Abstract

We introduce 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, thereby improving the result.
A specific example (BD + 70°68) is worked out. The configuration of
reference stars is also discussed.

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