HLIRGS, An X-ray view
The ultraluminous state refined: spectral and temporal characteristics of super-Eddington accretion Tim Roberts Andy Sutton (Durham) Matt Middleton (Cambridge)
Chandra X-Ray Observatory CXC Paul Plucinsky February 2005 1 A Comparison of Spectral Fit Results of E0102 from the Chandra and XMM CCDs Paul Plucinsky.
NASSP Masters 5003F - Computational Astronomy - 2009 Lecture 23 Two areas of my current research interest: –Parallel CLEAN. –Looking for bursts in XMM.
The Environments of Galaxies: from Kiloparsecs to Megaparsecs August 2004 Cool Cores in Galaxy Groups Ewan O’Sullivan Harvard-Smithsonian Center for Astrophysics.
Background .
Cool Cores in Galaxy Groups
Formation and Evolution of Early-Type Galaxies in clusters Yara Jaffé 1,2 Alfonso Arag Ó n-Salamanca 1 1. The University of Nottingham 2. European Southern.
Group Evolution Multi-wavelength Survey (GEMS) Duncan A. Forbes Centre for Astrophysics & Supercomputing, Swinburne University.
Galaxy groups Michael Balogh Department of Physics and Astronomy University of Waterloo.
X-RAY GROUPS WITH CHANDRA AND XMM: MASS, ENTROPY AND AGN HEATING
Tiziana Di Salvo DSFA Università di Palermo
