Hostname: page-component-5c6d5d7d68-sv6ng Total loading time: 0 Render date: 2024-08-29T19:02:05.599Z Has data issue: false hasContentIssue false
  • English
  • Français

On the total kinetic energy of our Galaxy with the contribution of the populations

Published online by Cambridge University Press:  07 August 2017

S. Ninković
S. Ninković*
Affiliation:
Astronomical Observatory Volgina 7 11050 Beograd Yugoslavia

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 total kinetic energy of our Galaxy is estimated to be (0.55 – 3.3) x 1016M⊙km2s–2 and the specific one to about 4 × 104km2s–2.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 464
Copyright
Copyright © Kluwer 

References

1. Freeman, K. C. (1987) ‘The Galactic Spheroid and Old Disk’, Annual Review of Astronomy and Astrophysics 25, 603–632.Google Scholar
2. Blanco, V. and Terndrup, D. M. (1989) ‘Longitude Distribution of Bulge M Giants: the Mass and Large-Scale Structure of the Spheroid’, Astronomical Journal 98, 843–852.CrossRefGoogle Scholar
3. Carney, B. W., Latham, D. W. and Laird, J. B. (1990) ‘A Survey of Proper-Motion Stars.X. The Early Evolution of the Galaxy's Halo’, Astronomical Journal 99, 572–589.Google Scholar