Clusters of galaxies are gravitationally bound configurations containing typically hundreds of
galaxies in a region about 10 25 cm in size. They range from irregular clusters, with strong …

The hot gas in the cores of rich galaxy clusters is metal-rich with nearly solar abundances of
metals. It is not clear whether the metals were shed from galaxies via protogalactic winds or …

Analysis of spatially resolved ASCA spectra of the intracluster gas in Abell 496 confirms
there are mild metal abundance enhancements near the center, as previously found in a …

One of the biggest open questions regarding the evolution of the galaxy population over
time, is how their properties (such as their morphologies) are affected by their local …

The purpose of this study was to determine whether there was consensus among general
education teachers, special education teachers, and educational interpreters regarding their …

X-ray line observations of clusters of galaxies have shown that the X-ray emission in clusters
is mainly thermal emission from hot diffuse gas, and that much of this gas has come out of …

The calculations presented suggest that the material stripped from galaxies and gathered in
wakes in a rich cluster can only begin to mix efficiently with the surroundings if galaxies …

The hot gas in the cores of rich galaxy clusters is metal-rich with nearly solar abundances of
metals. It is not clear whether the metals were shed from galaxies via protogalactic winds or …

We analyze the Ginga LAC and Einstein SSS spectra of four cooling flow clusters, A496,
A1795, A2142 and A2199, each of which shows firm evidence of a relatively cool …

This dissertation presents the analysis of spatially resolved ASCA satellite X-ray spectra for
four clusters of galaxies (Abell 496, Abell 2199, Abell 3571 and Abell 1060). The abundance …