http://arxiv.org/abs/1405.2070
The ultra-deep multiwavelength HST Frontier Fields coverage of the Abell Cluster 2744 is used to derive the stellar population properties of its intra-cluster light (ICL). The restframe colors of the ICL of this intermediate redshift (z=0.3064) massive cluster are bluer (g-r~0.7; i-J~0.6) than those found in the stellar populations of its main galaxy members (g-r~0.85; i-J~0.75). Based on these colors, we derive the following mean metallicity Z~0.018+-0.003 for the ICL. The ICL age is ~3-5 Gyr younger than the average age of the massive galaxies of the cluster. The fraction of stellar mass in the ICL component comprises at least 6% of the total stellar mass of the galaxy cluster. Our data is consistent with a scenario where the bulk of the ICL of Abell 2744 has been formed relatively recently (z<1). The stellar population properties of the ICL suggest that this diffuse component is mainly the result of the disruption of infalling galaxies with similar characteristics in mass (M*~3×10^{10} Msun) and metallicity than our own Milky Way.
M. Montes and I. Trujillo
Mon, 12 May 14
27/40
Comments: 2 figures, ApJ Letter submitted. Comments are welcome
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