Abstract
Owing to the fact that the near future should see a rapidly expanding set of probes of the halo masses of individual early-type galaxies, we introduce a convenient parameter for characterizing the halo masses from both observational and theoretical results: del(l)Y the logarithmic radial gradient of the mass-to-light ratio. Using halo density profiles from Delta-cold dark matter (CDM) simulations, we derive predictions for this gradient for various galaxy luminosities and star formation efficiencies SF. As a pilot study, we assemble the available del(l)Y data from kinematics in early-type galaxies - representing the first unbiased study of halo masses in a wide range of early-type galaxy luminosities - and find a correlation between luminosity and del(l)Y, such that the brightest galaxies appear the most dark-matter dominated. We find that the gradients in most of the brightest galaxies may fit in well with the CDM predictions, but that there is also a population of fainter galaxies whose gradients are so low as to imply an unreasonably high star formation efficiency epsilon(SF) > 1. This difficulty is eased if dark haloes are not assumed to have the standard CDM profiles, but lower central concentrations.
Original language | English |
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Pages (from-to) | 691-706 |
Number of pages | 16 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 357 |
Issue number | 2 |
DOIs | |
Publication status | Published - 21-Feb-2005 |
Keywords
- galaxies : evolution
- galaxies : fundamental parameters
- galaxies : haloes
- galaxies : kinematics and dynamics
- dark matter
- DIGITAL SKY SURVEY
- DARK-MATTER HALOS
- GLOBULAR-CLUSTER SYSTEM
- INFRARED FUNDAMENTAL PLANE
- DWARF SPHEROIDAL GALAXIES
- LAMBDA-CDM UNIVERSE
- ELLIPTIC GALAXIES
- VELOCITY DISPERSION
- STELLAR POPULATION
- SPIRAL GALAXIES