PPT-Anatomy of the AGN in NGC 5548: Discovery of a fast and massive outflow

Jelle Kaastra Jerry Kriss Massimo Cappi Missagh Mehdipour PierreOlivier Petrucci Katrien Steenbrugge Nahum Arav Ehud Behar Stefano Bianchi Rozenn Boissay. 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. Are They Chemically Distinct to Their Fellow RGB and HB Stars?. M5: SDSS . Simon . Campbell. 1. . Universitat. . Politecnica. de . Catalunya. , Barcelona, Spain. 2. CSPA, . Monash. University, Melbourne, Australia. は階層的銀河形成論で説明. できるか？. Motohiro. 　. Enoki. Tomoaki Ishiyama (Tsukuba Univ.). Masakazu A. R. Kobayashi (Ehime Univ.). Masahiro . Nagashima. . (Nagasaki Univ. .). §1. Introduction. 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 . Andrei LobanovMPIfR, Bonn AGN/RG ScienceAGN/RG Science AGN/RG drivers for LOFAR and SKA: astrophysical masers, nuclear regions of AGN, physics of relativistic and mildly relativistic outflows, kinetic Guido Risaliti. INAF – . Osservatorio. . Astrofisico. . di. Arcetri & . Harvard-Smithsonian Center for Astrophysics. M. . Polletta. ;. Urry. & . Padovani. 1995. Unified models: History. Stephen R. Ash, MD, FACP. Nephrology, Indiana University Health Arnett, and Ash Access Technology, Lafayette, Indiana. . ASDIN Blog Entry. 2016. Patient History and first outflow failure with inflow pain . in the Milky Way. Christian Johnson. Smithsonian Astrophysical Observatory. “Typical” Globular Clusters. Main Sequence. Main Sequence Turn-off. Subgiant Branch. Red Giant Branch. Horizontal Branch. Q. . Daniel . Wang . University . of . Massachusetts. We will be able to better trace the . f. eedback . from . stars and/. or . AGNs and its role in shaping galaxy ecosystem by breaking various degeneracies.. Eric D. . Rappin. , Michael C. Morgan, and Gregory J. Tripoli. J. Atmos. Sci., Volume 68, February 2011. ATM 527 Paper Discussion. Patrick Duran. 3/3/2014. Thoughts?. Motivation. TC environment is known to have an influence on TC structure and intensification. C. Jerry Lin. *. 1,. . Li Pan. 1. , David G. Streets. 2. , Suraj Shetty. 1. , Carey Jang. 3. , Joshua Fu. 4. , Thomas C. Ho. 1. , Hsing-wei Chu. 1. 1 . College of Engineering, Lamar University, Beaumont, TX. Seyfert. Galaxies Ark 564 and . Mrk. 590. Anjali. Gupta. Columbus State . Ohio State University. Collaborators: . Smita. . Mathur. , . Yair. . Krongold. Low velocity outflows are ubiquitous. . Stephen R. Ash, MD, FACP. Nephrology, Indiana University Health Arnett, and Ash Access Technology, Lafayette, Indiana. . ASDIN Blog Entry. 2016. Patient History and first outflow failure with inflow pain . 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 .