Abstract
In a program conducted to isolate AGK3 stars with large proper motions, it has been found that more than one hundred stars seem to be affected by large errors in their published proper motions. For some of those objects south of +25 degrees, new proper motions are being obtained using, as first-epoch positions, the published material of the Astrographic Catalogue. Second-epoch positions are derived from new plates taken with the Yale Southern Observatory double astrograph.
Similar content being viewed by others
References
Giclas, H.L., Burnham, R., Thomas, N.G. (1971). ‘Lowell Proper Motions Survey (nothern hemisphere) The G Numbered Stars’. Lowell Observatory.
Lopez, C.E. (1986).IAU Inf. Bull. Var. Stars No.2864.
Lopez, C.E., Cesco, M.R. (1986).IAU Inf. Bull. Var. Stars No.2940.
Lopez, C.E., Sanguin, J. G. (1987a).IAU Inf. Bull. Var. Stars. No.3023.
Lopez, C.E., Sanguin, J.G. (1987b). (in preparation).
Lopez, C.E., Torres, J.E. (1987).IAU Inf. Bull. Var. Stars No.2980.
Luyten, W.J. (1979). ‘NLTT Cataloque’, Minneapolis, Minnesota.
Stephenson, C. B. (1978).Astron. J. 83, 816.
Stephenson, C.B. Hulbert, S.J. (1984).Astron. J. 89, 1261.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Lopez, C.E. New proper motions for some AGK3 stars. Astrophys Space Sci 177, 73–77 (1991). https://doi.org/10.1007/BF00643656
Issue Date:
DOI: https://doi.org/10.1007/BF00643656