Parallaxes and proper motions. XIV

Details Parallaxes and proper motions. XIV Parallaxes and proper motions. XIV

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..141b&link_type=abstract

Astronomical Journal, vol. 87, Jan. 1982, p. 141-144.

Astronomy and Astrophysics

Astronomy

5

Astronomical Photography, Stellar Motions, Stellar Parallax, Data Reduction, Photographic Plates, Stellar Magnitude

Scientific paper

Since earlier parallax solutions have shown that reductions made by means of linear plate constants do not vary significantly from those using the iterative central overlap technique, the former is used to compute the parallaxes and proper motions for 19 stars to the nearest ten-thousandth of an arcsec and separately in X and Y coordinates, along with a combined solution. These methods follow the recommendations and practices of such recent investigators as Lutz and Upgren (1980) and Upgren and Breakiron (1981).

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