Key points are not available for this paper at this time.
Based on a uniform dynamical analysis of line-profile shapes for 21 luminous round elliptical galaxies, we have investigated the dynamical family relations of ellipticals: (i) The circular velocity curves (CVCs) of elliptical galaxies are flat to within ~10% for R>~0. 2Rₑ. (ii) Most ellipticals are moderately radially anisotropic; their dynamical structure is surprisingly uniform. (iii) Elliptical galaxies follow a Tully-Fisher (TF) relation, with vcᵐax=300 km/s for an LB^* galaxy. At given vcᵐax, they are ~1 mag fainter in B and appear to have slightly lower baryonic mass than spirals even for maximum M/LB. (iv) The luminosity dependence of M/LB is confirmed. The tilt of the Fundamental Plane is not caused by dynamical non-homology, nor only by an increasing dark matter fraction with L. It is, however, consistent with stellar population models based on published metallicities and ages. The main driver is therefore probably metallicity, and a secondary population effect is needed to explain the K-band tilt. (v) These results make it likely that elliptical galaxies have nearly maximal M/LB (minimal halos). (vi) Despite the uniformly flat CVCs, there is a spread in cumulative M/LB (r). Some galaxies have no indication for dark matter within 2Rₑ, whereas others have local M/LBs of 20-30 at 2Rₑ. (vii) In models with maximum stellar mass, the dark matter contributes ~10-40% of the mass within Rₑ. (viii) The corresponding halo core densities and phase-space densities are at least ~25 times larger and the halo core radii ~4 times smaller than in spiral galaxies of the same vcᵐax. The increase in M/L sets in at ~10 times larger acceleration than in spirals. This could imply that elliptical galaxy halos collapsed at high redshift or that some of the dark matter in ellipticals might be baryonic. (abridged)
Gerhard et al. (Sun,) studied this question.