Results of the Herstmonceux parallax programme. III

Astronomy and Astrophysics – Astronomy

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Astronomical Catalogs, Spectroscopic Analysis, Stellar Parallax, Astronomical Coordinates, Astronomical Photometry, Correlation, Errors

Scientific paper

Herstmonceux parallaxes measured with the 26-in. refractor for 28 stars are presented. Parameters examined include photometric V and B magnitudes to 0.01 mag or approximate visual and photographic magnitudes to 0.1 mag; the approximate effective photographic magnitude; the parallax weights of the right ascension and combined solutions; the relative parallax solutions and their standard errors; and the adopted parallax, absolute magnitude, and the positive and negative range corresponding to the standard error of the relative parallax. A weak correlation appears to exist between the relative parallax solutions and right ascension. Though the phase is similar to that obtained by Thomas (1973), the variation is much smaller. Both the phase and the amplitude of the relative parallax solutions are approximately the same as those obtained by Lippincott (1971).

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