XMM-Newton and Chandra combined analysis of the most massive galaxy clusters at z~1
We present a detailed study of the spatially resolved thermodynamic and hydrostatic mass profiles of the five most massive clusters detected at z~1 via the...
The standard model of cosmology is based on the Friedmann-Robertson-Walker (FRW) metric. Often written in terms of co-moving coordinates, this elegant and...
Despite being some of the most abundant elements in the Universe the determination and understanding of the chemical evolution of C and N is still very...