Astrometric parameters of visual double stars derived from simulated HIPPARCOS measurements

Details Astrometric parameters of visual double stars derived from simulated HIPPARCOS measurements Astrometric parameters of visual double stars derived from simulated HIPPARCOS measurements

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142..161b&link_type=abstract

(IAU, Colloquium on Wide Components in Double and Multiple Stars, 97th, Brussels, Belgium, June 8-13, 1987) Astrophysics and Spa

Astronomy and Astrophysics

Astrophysics

Astrometry, Double Stars, Hipparcos Satellite, Visible Spectrum, Correlation Coefficients, Stellar Systems

Scientific paper

In the course of the reduction of Hipparcos data the astrometric parameter determination of visual binaries is reduced to the parameter determination of single stars. This approach assumes that the off-set of the binary components with respect to the conventional light point directly measured by the Hipparcos telescope are known on the individual scanning circles. The computer algorithms are outlined, preliminary results based on simulated measurements are discussed.

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