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Moments of peculiar velocities in stellar systems by point axial symmetry
Published online by Cambridge University Press: 07 August 2017
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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