Chaos and the Shapes of Elliptical Galaxies
Astrophysics
2009-10-28 v1
Abstract
Hubble Space Telescope (HST) observations reveal that the density of stars in most elliptical galaxies rises toward the center in a power-law cusp. Many of these galaxies also contain central dark objects,possibly supermassive black holes. The gravitational force from a steep cusp or black hole will destroy most of the box orbits that constitute the ``backbone'' of a triaxial stellar system. Detailed modelling demonstrates that the resulting chaos can preclude a self-consistent, strongly triaxial equilibrium. Most elliptical galaxies may therefore be nearly axisymmetric, either oblate or prolate.
Cite
@article{arxiv.astro-ph/9601091,
title = {Chaos and the Shapes of Elliptical Galaxies},
author = {David Merritt},
journal= {arXiv preprint arXiv:astro-ph/9601091},
year = {2009}
}
Comments
10 TEX pages, 3 PostScript figures, uses AASTEX, epsf.sty. To appear in SCIENCE, January 19, 1996