Hostname: page-component-848d4c4894-8bljj Total loading time: 0 Render date: 2024-06-26T04:50:04.739Z Has data issue: false hasContentIssue false

Trigonometric Parallaxes Obtained with the UK Schmidt Telescope

Published online by Cambridge University Press:  04 August 2017

C A Murray
Affiliation:
Royal Greenwich Observatory
P M Corben
Affiliation:
Royal Greenwich Observatory
R W Argyle
Affiliation:
Royal Greenwich Observatory

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In continuation of a long term programme of measurement of parallaxes and proper motions in the South Galactic Cap from plates taken with the UK Schmidt Telescope and measured in GALAXY at RGO, data for some 800 red stars brighter than B = 17.5 have been derived from two independent plate series. The parallaxes obtained from unfiltered IIaO plates show a large systematic error depending on magnitude compared with those obtained from IIaD plates with GG 495 filter. After correction, the combined trigonometric parallaxes show very satisfactory agreement with photometric parallaxes, and the average r.m.s. error of a combined parallax is found to be about ±0″.012 both from internal and external evidence.

Type
III. Photographic Astrometry
Copyright
Copyright © Reidel 1986 

References

Alexander, J. B., Jones, D. H. P. and Sinclair, J. E., 1983 RGO Bull. 191.Google Scholar
Eggen, O. J., 1976a Astrophys. J. 204, 101.Google Scholar
Eggen, O. J., 1976b Astrophys. J. Suppl. 30, 351.CrossRefGoogle Scholar
Jones, D. H. P., Sinclair, J. E. and Alexander, J. B., 1981, Mon. Not. R. astr. Soc., 194, 403.CrossRefGoogle Scholar
Murray, C. A. and Corben, P. M. 1979 Mon. Not. R. astr. Soc., 187, 723.CrossRefGoogle Scholar