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Point-axial mass distribution in the external Galactic Bulge

  • J. Sanz-Subirana (a1) and J.M. Juan-Zornoza (a2)

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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.

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Copyright

References

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

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