On the deprojection of triaxial galaxies with St\"ackel potentials
Abstract
A family of triaxial St\"ackel potential-density pairs is introduced. With the help of a Quadratic Programming method, a linear combination of potential-density pairs of this family which fits a given projected density distribution can be built. This deprojection strategy can be used to model the potentials of triaxial elliptical galaxies with or without dark halos. Besides, we show that the expressions for the St\"ackel triaxial density and potential are considerably simplified when expressed in terms of divided differences, which are convenient numerically. We present an example of triaxial deprojection for the galaxy NGC~5128 whose photometry follows the de Vaucouleurs law.
Keywords
Cite
@article{arxiv.astro-ph/9603065,
title = {On the deprojection of triaxial galaxies with St\"ackel potentials},
author = {A. Mathieu and H. Dejonghe},
journal= {arXiv preprint arXiv:astro-ph/9603065},
year = {2007}
}
Comments
8 pages, to appear in A&A, postscript file with figures available at ftp://naos.rug.ac.be/pub/deprojection.ps.Z