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:
Post a Comment