PPT-Probing AGN physics

with VLBI at Parkes Stas Shabala University of Tasmania Why study AGN AGN physics Brightest objects in the Universe yet we dont know Composition Accretion outflow connection Details of interaction with environment. 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. and . Galaxy Evolution. Meg Urry. Yale University. ~All galaxies host supermassive black holes. The . formation. and . evolution. of . galaxies. is closely tied to. the . growth. of . black holes. Harry Ferguson (STScI). Feedback. Behroozi. + 2011. Halo quenching. Quasar mode AGN. Radio Mode AGN. (. SNe. ). SNe. Satellites: Ram pressure, tides, shocks…. UV back-ground. AGN feedback in . SAMs. Ioana. . Duţ. an. Advisors: Peter Biermann & Alan Roy. Phinney, 1994. Large-scale mechanisms: . . bar potentials. & galaxy interactions. . THEORY: . Gaseous orbits in a weak bar potential: . 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. Violette Impellizzeri (NRAO). Alan Roy (. MPIfR. ), Christian Henkel (. MPIfR. ). The unified scheme of AGN. Diversity of AGN classes explained by a single unified scheme :. The nuclear activity is powered by a . 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). Chris Packham. University of Texas at San Antonio. Outline. Polarization processes of importance to AGN. Scattering. Dichroism. Synchrotron. Sy’s. and BLs. MHD & the torus. Conclusions. Caveats: This review talk is being far from comprehensive, and rather focuses on some topics that I’ve enjoyed reading of late – sorry to all those I offend by not featuring their great work. Hee. -Won Lee. Department of Physics and Astronomy. Sejong. University. 2015. 1. 27. Content. Introduction. Scattering . and Unification of AGN. Scattered Ly . alpha. Balmer. Wings. Discussion. Active Galactic Nuclei. VG. So we want a color magnitude diagram for AGN so that by looking at the color of an AGN we can get its luminosity. But AGN have no fusion, why would we expect a color-magnitude relation?. The gas that accretes onto the black hole is still hot and so must follow the Blackbody Radiation law. . Carisa Petris, Don Liu . Issue . 7. , 2017. A presentation to:. Meeting name. Date. Table of Contents. 01. Background. 02. Types. of studies. 03. Key results. 04. Tables (Risk of Bias/Forest Plots). Learn how to excel in AP Physics with this comprehensive guide. Explore essential concepts, study strategies, and resources to ace your AP Physics exam. Purdue University. (currently on sabbatical at Univ. College Cork, Ireland). Matthew Lister. VLBA. Fermi. UMRAO. OVRO. Chandra. MOJAVE Collaborators. M. Lister (P.I.), N. Cooper, B. Hogan, S. . Kuchibhotla.