We also show the calculated x-ray intensity for a range of atmospheric abundances for Jupiter and Saturn and for a number of solar irradiance spectra. The model calculations are compared with recent x-ray observations of Jupiter and Saturn.

The underlying procedure was revised and extended in the scope of this work to suit the purpose of a default correction tool. A script package was developed to largely automate the necessary steps for validation purposes and future updates.

We present an analysis of X-ray and UV data obtained with the XMM-Newton Observatory of the long-period dwarf nova RU Peg.

Covered: Physics in the core of clusters; Physics of merger events; The dark matter content and distribution; The role of non-gravitational processes and the ICM enrichment; Observation of high z clusters and the evolution of cluster ...

The first half of this book introduces the history of high-resolution X-ray spectroscopy and different generations of X-ray spectrometers.