Abstract
In this paper, we make use of the Stumpff's functions to solve the problem of determining the orbit of a visual binary star in universal variables. The method is thus valid for all types of orbits: hyperbolic, parabolic and elliptic.
Similar content being viewed by others
References
Aitken, R.G.: 1935,The Binary Stars, 2nd ed., McGraw-Hill, New York.
Cid, R.: 1958,Astron. J., 63, n° 9, 395.
Cid, R.: 1964,Rev. Acad. Cienc. Zaragoza XVIII.
Correas, J.M.: 1974,Rev. Acad. Cienc. Zaragoza XXIX, 129.
Correas, J.M.: 1976,Astron. Astrophys. 51, 423.
Danby, J.M.A.: 1988,Fundamentals of Celestial Mechanic, 2nd edition. Wilmann-Bell, Richmond.
Deprit, A., Felipe, A., and Ferrer, S.: 1994,Celest. Mech. & Dyn. Astron. 58, 151.
Docobo, J.A.: 1985,Celes. Mech. 36, 143.
Dommanget, J.: 1978,Astron. Astrophys. 68, 315.
Dommanget, J.: 1981,Astron. Astrophys. 94, 45.
Stumpff, K.: 1947,Astron. Nach. 275, 108.
Stumpff, K.: 1965,Himmelsmechanick, Deutcher. Verlag der Wissenschaften.
Thiele, T.N.: 1883,Astron. Nach. 104, 245.
Viñuales, E.: 1993,Generalización de métodos de cálculo y corrección de órbitas de estrellas dobles visuales, Ph. D. dissertation. Univ. Zaragoza.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Viñuales, E., Cid, R. & Elipe, A. Visual binary star orbits in universal variables. Astrophys Space Sci 229, 117–127 (1995). https://doi.org/10.1007/BF00658570
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF00658570