Slide 1 HOT TIMES FOR COOLING FLOWS Mateusz Ruszkowski Slide 2 Cooling flow cluster Non-cooling flow cluster gas radiates X-rays & loses pressure support against gravity…

Slide 1 Slide 2 OUTLINE X-RAY STATES & RADIO JETS (BLACK HOLES) Radio phenomenology vs accretion modes LUMINOSITY CORRELATIONS (BLACK HOLES) radio/X-ray NIR/X-ray dependence…

Françoise Combes February 13, 2014 AGN-driven outflows * Perseus cooling flow Mrk 231 * Gaibler et al 2011 Inefficient star formation Behroozi et al 2013 * MS0735.6+7421…

Demography of supermassive black holes: mergers & gravitational waves Françoise Combes Observatoire de Paris Monday 9 November Overview 1- Co-evolution of galaxies and…

Françoise Combes February 13, 2014 AGN-driven outflows * Perseus cooling flow Mrk 231 * Gaibler et al 2011 Inefficient star formation Behroozi et al 2013 * MS0735.6+7421…

Colorectal Trauma Colorectal Conference St Luke’s-Roosevelt Hospital Department of Surgery Leslie Tyrie, PGY III 16 March 2006 Colorectal Anatomy Right Colon, Left Colon,…

HOT TIMES FOR COOLING FLOWS Mateusz Ruszkowski Cooling flow cluster Non-cooling flow cluster gas radiates X-rays & loses pressure support against gravity gas sinks towards…

The X-ray mirrors Giovanni Miniutti Institute of Astronomy, University of Cambridge SIMBOL-X - 2007 May -Bologna Accreting BHs: main spectral components Soft excess Power…

NASSP Masters 5003F - Computational Astronomy - 2009 Lecture 21 6.4 keV Fe line and the Kerr metric Satellite observatories Attitude and boresight X-ray instrumentation and…

Simulating the SZ Sky Predictions for Upcoming Sunyaev-Zel’dovich Effect Galaxy Cluster Surveys Eric J. Hallman CASA, University of Colorado 16 February, 2007 Clusters…