Titlebook: Soft X-Ray Emission from Clusters of Galaxies and Related Phenomena; Richard Lieu,Jonathan Mittaz Conference proceedings 2004 Springer Sci

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Soft (1 KEV) X-Ray Emission in Galaxy Clusterswe find evidence of a soft excess that can be modeled either as thermal emission or as non-thermal emission. For IC 1262, the thermal interpretation is nonphysical and the non-thermal model has further support from a radio halo that we propose exists in the cluster center. For Abell 754, we modeled

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XMM-Newton Discovery of O VII Emission from Warm Gas in Clusters of Galaxiesbuted to the Warm-Hot Intergalactic Medium. The original sample of clusters studied for this purpose has been extended and two more clusters with a soft X-ray excess have been found. We discuss the physical properties of the warm gas, in particular the density, spatial extent, abundances and tempera

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The Fuse Survey of O VI in the Galactic Haloc objects and two distant halo stars are analyzed to obtain measures of O VI absorption along paths through the Milky Way thick disk/halo. Strong O VI absorption over the velocity range from —100 to 100 km s. reveals a widespread but highly irregular distribution of O VI, implying the existence of s

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