Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds

Details Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds

2009-07-22

arxiv.org/abs/0907.3800v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

9 pages, 6 figures, accepted by A&A

Scientific paper

We investigate the efficiency and time-dependence of thermally and cosmic ray driven galactic winds for the metal enrichment of the intra-cluster medium (ICM) using a new analytical approximation for the mass outflow. The spatial distribution of the metals are studied using radial metallicity profiles and 2D metallicity maps of the model clusters as they would be observed by X-ray telescopes like XMM-Newton. Analytical approximations for the mass loss by galactic winds driven by thermal and cosmic ray pressure are derived from the Bernoulli equation and implemented in combined N-body/hydrodynamic cosmological simulations with a semi-analytical galaxy formation model. Observable quantities like the mean metallicity, metallicity profiles, and 2D metal maps of the model clusters are derived from the simulations. We find that galactic winds alone cannot account for the observed metallicity of the ICM. At redshift $z=0$ the model clusters have metallicities originating from galactic winds which are almost a factor of 10 lower than the observed values. For massive, relaxed clusters we find, as in previous studies, a central drop in the metallicity due to a suppression of the galactic winds by the pressure of the ambient ICM. Combining ram-pressure stripping and galactic winds we find radial metallicity profiles of the model clusters which agree qualitatively with observed profiles. Only in the inner parts of massive clusters the observed profiles are steeper than in the simulations. Also the combination of galactic winds and ram-pressure stripping yields too low values for the ICM metallicities. The slope of the redshift evolution of the mean metallicity in the simulations agrees reasonably well with recent observations.

Affiliated with

Also associated with

No associations

Rating

Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metal enrichment of the intra-cluster medium by thermally and cosmic-ray driven galactic winds will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-128050