Axisymmetric galactic models in spherical potentials

Details Axisymmetric galactic models in spherical potentials Axisymmetric galactic models in spherical potentials

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.225..107h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 225, no. 1, p. 107-115

Astronomy and Astrophysics

Astrophysics

Dark Matter, Galactic Mass, Galactic Rotation, Galactic Structure, Galaxies, Kinematics, Symmetry, Angular Momentum, Density (Mass/Volume), Line Of Sight, Mass Distribution, Stellar Models, Velocity Distribution

Scientific paper

We study projected kinematic characteristics of a class of axisymmetric models for the luminous components of galaxies. Models of this class are known as extended Osipkov-Merritt models and have been studied first by Arnold (1990). The line-of-sight velocity dispersions are given and the profiles of the projected velocity distribution are described using their Gauss-Hermite moments.

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