Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-16564
Ferreras, I; Saha, P; Burles, S (2008). Unveiling dark haloes in lensing galaxies. Monthly Notices of the Royal Astronomical Society, 383(3):857-863.
- Registered users only
View at publisher
We present a spatially resolved comparison of the stellar mass and total mass surface distributions of nine early-type galaxies. The galaxies are a subset of the Sloan Lens ACS Survey. The total mass distributions are obtained by exploring pixelated mass models that reproduce the lensed images. The stellar mass distributions are derived from population-synthesis models fit to the photometry of the lensing galaxies. Uncertainties – mainly model degeneracies – are also computed. Stars can account for all the mass in the inner regions. A Salpeter initial mass function actually gives too much stellar mass in the inner regions and hence appears ruled out. Dark matter becomes significant by the half-light radius and becomes increasingly dominant at larger radii. The stellar and dark components are closely aligned, but the actual ellipticities are not correlated. Finally, we attempt to intuitively summarize the results by rendering the density, stellar versus dark ratio, and uncertainties as false-colour maps.
23 downloads since deposited on 26 Feb 2009
7 downloads since 12 months
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Dewey Decimal Classification:||530 Physics|
|Deposited On:||26 Feb 2009 14:59|
|Last Modified:||27 Nov 2013 23:35|
|Additional Information:||The definitive version is available at www.blackwell-synergy.com|
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page