The Origin of Metals in the Circumgalactic and the
University of California, Santa Cruz
The distribution and evolution of metals in the circumgalactic medium (CGM) and the intergalactic medium (IGM) are “fossil records” of the interactions between galaxies and their surrounding gas. In this
talk, I will first discuss the modeling of metal enrichment in cosmological simulations, focusing on the treatment of supernova-driven outflows, metal cooling and metal mixing due to turbulence.
Then I will present a detailed study of the metal-enriched CGM of a massive galaxy at z = 3, using results from a series of cosmological hydrodynamic “zoom-in” simulations. Our study shows that: 1) metal
enriched gas extends as far as 200 physical kpc (more than 4 virial radii) from the host galaxy center; 2) metals located farther away from the host are generally produced at an earlier epoch; 3) there
are three sources of heavy elements: the main host, its satellite progenitors and its dwarf companions, and the latter two contribute significantly to the metal budget. Finally, I will present a comparison between simulations and recent observations on spatial distribution of metal absorbers (such as C IV, C II, Si IV and Si II) around Lyman break galaxies at z = 2-3, and discuss the effects of feedback models and metal cooling.
|Date: ||Thursday, 15 December 2011|
|Where: ||Université de Montréal|
| ||Pavillon Roger-Gaudry, local D-460|
|Contact: ||Marie-Eve Naud|