PPT-Microphysics and X-ray Spectra of AGN Outflows

Author : cheryl-pisano | Published Date : 2016-09-06

T Kallman NASAGSFC Line emission efficiency across the spectrum Thermal stability The broadband spectrum of active galaxies flat over 68 decades Very different from

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Microphysics and X-ray Spectra of AGN Outflows: Transcript

T Kallman NASAGSFC Line emission efficiency across the spectrum Thermal stability The broadband spectrum of active galaxies flat over 68 decades Very different from stars Most are strong Xray sources. . Statistics. : . 1.8 . Ms. ½. . sq. .deg. . @. 160 . ksec. 1761 . sources. Dec. ’06-June ’07. Catalog. : . Elvis . et. al., . 2009, ApJS 184, 158. Martin Elvis, Francesca . Civano. , . Aldcroft. multitemperature. approach. . B. Sylwester, J. Sylwester, A. Kępa. . Space . Research. Centre, PAS, Wrocław, Poland. K.J.H. Phillips. Natural . History. . Museum. , London, UK. . V.D. . Kuznetsov. 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. with VLBI at . Parkes. Stas Shabala. University of Tasmania. Why study AGN. . AGN physics. Brightest objects in the Universe, yet we don’t know:. Composition. Accretion / outflow connection. Details of interaction with environment. 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. 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 Electra . Panagoulia. Institute of Astronomy, Cambridge, UK. W. ith: Andy Fabian. Jeremy Sanders. Julie . Hlavacek-Larrondo. X-ray View of Galaxy Ecosystems . 11. th. July 2014. RE J1034+396. Matthew Middleton. Spectral and timing similarities of AGN and . BHB. A simple scaling.... Index of -1.35 from analytical method (Vaughan et al. 2005) and large scale simulations (Middleton & Done 2010). 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. Nathalie . Japkowicz. , Colin . Bellinger. , . Shiven. Sharma, Rodney Berg, Kurt . Ungar. . University of Ottawa, Northern Illinois University. Radiation Protection Bureau, Health Canada. XRB. and . AGN. . Accretion . Processes. Anca. . Constantin. James Madison Univ.. W/. Paul . Green(SAO. ) . Tom . Aldcroft. (SAO. ). HongYan. . Zhou(USTChina. ). Daryl Haggard (. UWashington. ). Seyfert. Galaxies Ark 564 and . Mrk. 590. Anjali. Gupta. Columbus State . Ohio State University. Collaborators: . Smita. . Mathur. , . Yair. . Krongold. Low velocity outflows are ubiquitous. .

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