Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-23T14:41:53.629Z Has data issue: false hasContentIssue false

Point-axial mass distribution in the external Galactic Bulge

Published online by Cambridge University Press:  07 August 2017

J. Sanz-Subirana
Affiliation:
(1)Dept. de Matemàtica Aplicada i Telemàtica
J.M. Juan-Zornoza
Affiliation:
(2)Dept. de Física Aplicada Universitat Politècnica de Catalunya. Apdo. 30.002 - Barcelona. SPAIN EAN: [email protected]

Extract

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 main purpose in this work is to present some analytical results about the spatial distribution of the stars in the Galactic Bulge. These results have been obtained by considering that the stellar system verifies the collisionless Boltzman equation and the ellipsoidal hypothesis (non-axisymmetrical) for the distribution of peculiar velocities of the stars.

Type
Contributed Papers
Copyright
Copyright © Kluwer 1993 

References

1. Cubarsí, et al.: 1992, This Symposium.Google Scholar
2. Juan-Zornoza, J.M. et al.: 1991, Astrophys. Space Sci. 185, 95 Google Scholar
3. Sanz, J. et al.: 1987, Proc. IAU Twenty European Regional Astronomy Meeting 4, 227.Google Scholar
4. Chandrasekhar, S.: 1942, Principles of Stellar Dynamics, The University of Chicago Press, Chicago.Google Scholar
5. Sanz, et al.: 1989, Astrophys. and Space Sci. 156, 19.Google Scholar
6. Kinman, T.D. et al.: 1989, Astroph. J. 95, 804.Google Scholar
7. Rich, R.M.: 1992, Proc. IAU Symposium nd 149, 29.CrossRefGoogle Scholar
8. Sharples, R. et al.: 1990, M.N.R.S.A. 246, 54.Google Scholar
9. Ninkovich, S.: 1987, Astrophys. and Space Sci. 136, 299.CrossRefGoogle Scholar