Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-26T07:32:35.059Z Has data issue: false hasContentIssue false
  • English
  • Français

A study of the properties of galactocentric orbits

Published online by Cambridge University Press:  07 August 2017

A. A. Myullyari ,
Yu. V. Nechitajlov ,
S. Ninković  and
V. V. Orlov
A. A. Myullyari
Affiliation:
University of Petrozavodsk, USSR
Yu. V. Nechitajlov
Affiliation:
St Petersburg State University, 198904 Petrodvorets, Bibliotechnaya ploshchad' 2, USSR
S. Ninković
Affiliation:
Astronomical Observatory, Volgina 7, 11050 Beograd, Yugoslavia
V. V. Orlov
Affiliation:
St Petersburg State University, 198904 Petrodvorets, Bibliotechnaya ploshchad' 2, USSR

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.

The galactocentric motion of 14 stars from the solar neighbourhood is studied. The stars are divided into nine groups according to their heliocentric-velocity components. In this way one can follow the motion of the stars belonging to the same group in the past.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 461
Copyright
Copyright © Kluwer 

References

1. Gliese, W. (1969) ‘Catalogue of Nearby Stars’, Veroeffentlichungen des Astronomischen Rechen-Instituts, Heidelberg 22.Google Scholar
2. Sala, F. (1987) ‘Galactic Kinematics: An Axi-Symmetric Time-Depending Model with Separable Potential’, Rev. mex. astron. astrof. 14, 195–205.Google Scholar
3. Allen, C. and Martos, M. A. (1986) ‘A Simple Realistic Model of the Galactic Mass Distribution for Orbit Computations’, Revista mexicana de astronomia y astrofisica 13, 137–147.Google Scholar
4. Kutuzov, S. A. and Osipkov, L. P. (1989) ‘Dvukhkomponentnaya model' gravitatsionnogo polya Galaktiki’, Astronomicheskij zhurnal 66, 965–974.Google Scholar