Abstract
The orbital elements and masses of 12 wide visual double stars are determined by the Apparent Motion Parameters (AMP) method. These binaries are the following: ADS 48, 5983 (Delta Gem), 7251, 8002, 10329, 10386, 10759 (Psi Dra), 11061 (40/41 Dra), 11632, 12169, 12815 (16 Cyg) and 14636 (61 Cyg). Eight orbits are deduced by the first time. The observational basis of the investigation consists of: (1) 20–30 years long series of high accuracy positions obtained by photographic observations with the 26-inch refractor at Pulkovo, (2) accurate relative radial velocity of the components observed by the correlation method and (3) trigonometric parallaxes. These data provide the orbit calculations using AMP-method on the basis of very short arc of apparent tracks. The peculiarities of the AMP-method are considered.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsPreview
Unable to display preview. Download preview PDF.
References
A.A. Kisselev, O.V. Kiyaeva (1980) The method of Apparent Motion Parameters, used to determine the orbit elements of a visual double star on the basis of short arc observations, Astron. J. USSR, Vol. no. 57,p. 1227–1241 (in Russian).
L.G. Romanenko, E.L. Chentsov (1994) Determination of relative radial velocities of the components of visual binary stars from observations with the 6-meter telescope, Astron. J. USSR, Vol. no. 71,p. 278–281 (in Russian).
A.A. Tokovinin (1994) Radial velocities of the components of wide visual double stars, Astron. J. USSR, Vol. no. 71,p. 293–296 (in Russian).
A.A. Kisselev et al. (1994) Trigonometric parallaxes of 12 visual double star, Izvestia GAO at Pulkovo, No. 208, p. 9–17 (in Russian).
O.V. Kiyaeva (1983) Using old observations for correction of the visual double star orbit, Astron. J. USSR, Vol. no. 60,p. 1208–1216 (in Russian).
J. Hopmann (1955) Der Doppelstern ADS 11632, Mitt. Univ. Sternwarte Wien, Vol. no. 7, p. 67–82.
A.A. Tokovinin (1995) The multiple system ADS 11061, Pis’ma Astron. J. USSR, Vol. no. 21, p. 286–293 (in Russian).
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1997 Kluwer Academic Publishers
About this chapter
Cite this chapter
Kisselev, A.A., Kiyaeva, O.V., Romanenko, L.G. (1997). Visual Double Stars Orbits Obtained by Apparent Motion Parameters Method at Pulkovo. In: Docobo, J.A., Elipe, A., McAlister, H. (eds) Visual Double Stars: Formation, Dynamics and Evolutionary Tracks. Astrophysics and Space Science Library, vol 223. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1477-3_46
Download citation
DOI: https://doi.org/10.1007/978-94-009-1477-3_46
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7161-1
Online ISBN: 978-94-009-1477-3
eBook Packages: Springer Book Archive