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Moments of peculiar velocities in stellar systems by point axial symmetry

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

Extract

In this work we study a non-cylindrical point-axial symmetric stellar system model that verifies the Chandrasekhar postulates [1]. It explains the values for the centered moments of the peculiar velocities and the galactic rotation parameters, non possible with a cylindrical model [2].

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Copyright

References

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1. Chandrasekhar, S., 1942, “Principles of Stellar Dynamics”, Univ. of Chicago.
2. Sanz, J. et al., 1987, Proceedings of the 10th ERAM of the IAU.
3. Figueras, F. et al., 1987, IAU Colloquium No. 100, edited by Eichhorn, H.K. (Nac. Com. Astr., Belgrade).
4. Cubarsí, R., 1990, Astron. J. 99, 1558.

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