Hostname: page-component-77c89778f8-gq7q9 Total loading time: 0 Render date: 2024-07-18T22:23:27.111Z Has data issue: false hasContentIssue false

A Study of ADS 5983 (δ Geminorum)1

Published online by Cambridge University Press:  12 April 2016

Natalia A. Shakht
Affiliation:
Russian Academy of Sciences, Pulkovo, St. Petersburg 196140, Russia
Olga V. Kiyaeva
Affiliation:
Russian Academy of Sciences, Pulkovo, St. Petersburg 196140, Russia

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.

Regular photographic observations of ADS 5983 (δ Gem) with the Pulkovo 26-in refractor have been made since 1972. The series of observations over the time interval 1972-1990 are considered. New orbital elements of the binary are obtained by the AMP–method. Some wave with a period about 5 years in the orbital motion of this star is found.

Type
Classical Methods, Catalogs, & Databases
Copyright
Copyright © Astronomical Society of the Pacific 1992

Footnotes

1

The authors of this paper were unable to attend the Colloquium — eds.

References

Akhundova, G.V. & Guseynov, O.H. 1972, Astr. Circ. USSR, 728 Google Scholar
Batten, A.H. 1967, Sixth Catalogue of Orbital Elements of Spectroscopic Binary System, Publ. Dom. Astroph. Obs., 13, 8 Google Scholar
Blinnikov, S.I. & Ptitsyn, D.A. 1971, Astr. Circ. USSR, 663 Google Scholar
Hopmann, Y. 1959, Circ. D’Inform., 19 Google Scholar
Shakht, N.A. 1988, Pulkovo Obs. Izvestia, 205, 5 Google Scholar
Woolley, R., Eppe, E.A., Penston, M.J., & Pocock, S.B. 1970, Catalogue of Stars within 25 parsec of the Sun, Royal Obs. Annal 5Google Scholar