Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-41685
Tortora, C; Napolitano, N R; Romanowsky, A J; Jetzer, P (2010). Central dark matter trends in early-type galaxies from strong lensing, dynamics and stellar populations. Astrophysical Journal Letters, 721(1):L1-L5.
PDF (Accepted manuscript, Version 2)
PDF (Accepted manuscript, Version 1)
We analyze the correlations between central dark matter (DM) content of early-type galaxies and their sizes and ages, using a sample of intermediate-redshift (z ~ 0.2) gravitational lenses from the SLACS survey, and by comparing them to a larger sample of z ~ 0 galaxies. We decompose the deprojected galaxy masses into DM and stellar components using combinations of strong lensing, stellar dynamics, and stellar populations modeling. For a given stellar mass, we find that for galaxies with larger sizes, the DM fraction increases and the mean DM density decreases, consistently with the cuspy halos expected in cosmological formation scenarios. The DM fraction also decreases with stellar age, which can be partially explained by the inverse correlation between size and age. The residual trend may point to systematic dependencies on formation epoch of halo contraction or stellar initial mass functions. These results are in agreement with recent findings based on local galaxies by Napolitano et al. and suggest negligible evidence of galaxy evolution over the last ~2.5 Gyr other than passive stellar aging.
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Deposited On:||02 Mar 2011 09:32|
|Last Modified:||08 Jun 2014 17:15|
|Publisher:||Institute of Physics Publishing|
|Citations:||Web of Science®. Times Cited: 20|
Scopus®. Citation Count: 23
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