PPT-Studying AGN feedback in nearby X-ray groups and clusters

Electra Panagoulia Institute of Astronomy Cambridge UK W ith Andy Fabian Jeremy Sanders Julie HlavacekLarrondo Xray View of Galaxy Ecosystems 11 th July 2014. Fred Davies. ASTR 278. 2/23/12. Contents. Eddington Ratio. What does it mean?. How do we measure it?. Contents. Eddington Ratio. What does it mean?. How do we measure it?. Two regimes of measurement. Formation and cosmic evolution of massive black holes. Andrea Merloni. MPE, Garching. Syllabus. Monday:. Observational evidence of Supermassive Black Holes. AGN surveys. Tuesday: . The evolution of SMBH mass function and spin distributions. Formation and cosmic evolution of massive black holes. Andrea Merloni. MPE, Garching. Syllabus. Monday:. Observational evidence of Supermassive Black Holes. AGN surveys. Tuesday: . The evolution of SMBH mass function and spin distributions. . . . . MIR imaging & . s. pectroscopy. ISM dust model & PAH. . vectorized. Monte Carlo model . SED of a clumpy AGN torus. Frank . Heymann. (PhD), Martin Haas, . Endrik. . Kr. Capetti. , . R. Baldi, B. Balmaverde, S. Buttiglione. AGN 10 - Roma 10/09/2012. WHY AN AGN CENSUS?. A PROPER AGN CENSUS IS NEEDED FOR A VARIETY OF STUDIES, SUCH AS, . E.G.. , THE AGN/HOST GALAXY CONNECTION, THE PROPERTIES OF THE CENTRAL ENGINE, THE AGN LUMINOSITY FUNCTION . Nikos Fanidakis. and. C.M. Baugh, R.G. Bower, S. Cole, C. Done, C. S. . Frenk. 9. th. Hellenic Astronomical Conference, Athens, Greece September 20-24, 2009. Tiziana Venturi. . tventuri@ira.inaf.it. Active Galactic Nuclei 9 Ferrara, 27.05.2010. Radio VLBI . as. the . most. . direct. way . to. Studying in HE. What’s so different?. Session Outline. Session outline. Studying at university – some crucial differences and making the transition. How to study independently. Types of learning, teaching and assessments. a panchromatic view. Andrea Merloni. MPE. Merloni, FERO 8, September 2016. Introduction. What FERO is about:. Detailed physical . modelling. of the inner region of AGN. A few bright sources, lots of photons, extensive observational campaigns. reading your notes is NOT studying It is simply reOnly doing the readings for class is not studying It is simply doing the reading for class Re-reading leads to quick forgetting Ideas for active stud XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. ). Summary Talk. Craig . Sarazin. University of Virginia. Observations of radio halos, mini-halos and . relics – review - . Tiziana. . Venturi. Nice overview: . p. roperties of halos, relics, mini-halos. Jelle Kaastra. Jerry . Kriss. , Massimo . Cappi. , . Missagh. . Mehdipour. , Pierre-Olivier . Petrucci. , . Katrien. . Steenbrugge. , Nahum . Arav. , Ehud Behar, . Stefano . Bianchi, . Rozenn. . Boissay. Prof Chris Done. University . of Durham & ISAS/JAXA. AGN feedback. Magorrian-Gebhardt. relation gives BH mass!! Big black holes live in host galaxies with big bulges! Either measured by bulge luminosity or bulge mass (stellar velocity dispersion) or .