Wednesday, August 03, 2005


Adami et al. identify 17 groups in the Coma cluster by combining X-ray and galaxy redshift information.

Wittman et al. present first results from their cluster survey based on weak lensing.

Peterson et al. propose a new inference method for the ICM describing clusters as a collection of smoothed plasma particles with temperature, location, size, and abundances. X-ray data are predicted and iterated using MCMC.

Croton et al. investigate the growth of galaxies and SMBH using semi-analytic models on top of very large LCDM simulations.

No comments: