Potentials for stationary point-axial stellar system models

Details Potentials for stationary point-axial stellar system models Potentials for stationary point-axial stellar system models

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.185...95j&link_type=abstract

(IAU, European Astronomical Meeting, 12th, Davos, Switzerland, Oct. 8-11, 1990) Astrophysics and Space Science (ISSN 0004-640X),

Astronomy and Astrophysics

Astrophysics

1

Chandrasekhar Equation, Stellar Models, Stellar Rotation, Boltzmann Distribution, Mass Distribution, Stellar Systems

Scientific paper

A stellar system model that verifies the collisionless Boltzmann equation and the ellipsoidal hypothesis for the distribution of peculiar velocities of the stars is considered on the basis of the theory developed by Chandrasekhar (1942). The potential for such a model in a stationary state with point axial symmetry and with an equatorial plane of symmetry is determined. A spherical term which corresponds to the potential created inside a homogeneous sphere appears, accounting for the contribution of the galactic halo.

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