Wednesday, April 06, 2005


Reed et al. include gas cooling in high res N-body simulations and find small groups of galaxies can form by z~30 unless prevented by feedback processes.

Murray et al. present the results of their 5ksec deep Chandra survey of the 9.3 sq deg Bootes field.

Vikhlinin provides an algorithm to predict measured temperatures when actually observing a multi-component thermal plasma.

Keywords: clusters, AGN, star formation

No comments: