Abstract
We present the formulation of a new infinite family of self-consistent stellar models, designed to describe axisymmetric flat galaxies. The corresponding density-potential pair is obtained as a superposition of members belonging to the generalized Kalnajs family, by imposing the condition that the density can be expressed as a regular function of the gravitational potential, in order to derive analytically the corresponding equilibrium distribution functions (DFs). The resulting models are characterized by a well-behaved surface density, as in the case of generalized Kalnajs discs. Then, we present a study of the kinematical behaviour which reveals, in some particular cases, a very satisfactory behaviour of the rotational curves (without the assumption of a dark matter halo). We also analyse the equatorial orbit's stability, and Poincaré surfaces of section are performed for the three-dimensional orbits. Finally, we obtain the corresponding equilibrium DFs, using the approaches introduced by Kalnajs and Dejonghe. © 2008 The Authors.
Author supplied keywords
Cite
CITATION STYLE
Pedraza, J. F., Ramos-Caro, J., & González, G. A. (2008). An infinite family of self-consistent models for axisymmetric flat galaxies. Monthly Notices of the Royal Astronomical Society, 390(4), 1587–1597. https://doi.org/10.1111/j.1365-2966.2008.13846.x
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.