PPT-The MOJAVE AGN Program Dept. of Physics

Purdue University currently on sabbatical at Univ College Cork Ireland Matthew Lister VLBA Fermi UMRAO OVRO Chandra MOJAVE Collaborators M Lister PI N Cooper B Hogan S Kuchibhotla. . 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. JWST Workshop. – . STScI. Baltimore. June 8, 2011. Mid-Infrared Observation of High . Redshift. Galaxy Evolution. Most star formation activity occurs behind dust . Chary & Pope . 2011. Bouwens. . . . . 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. Tori. : . Theory & Observations. Moshe . Elitzur. . University of Kentucky . Unified Scheme for AGN. M. . ~ 10. 6 . – 10. 10. M. . R. s. ~ 10. 11 . – 10. 15 . cm. T. oroidal. 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. Establishing . a Tribally Owned . Service Provider. Sacred Wind Communications. The only non-tribally owned fully tribally-oriented telco. Our Mission: . to serve unserved tribal areas. . Our initial purpose: . 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. 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. 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. . Tamarisk Treatment in the Mojave River Watershed. Ken Lair. , Lair Restoration Consulting. Hesperia, CA. Chuck Bell and Jackie Lindgren. , . Mojave Desert Resource Conservation District. Victorville, CA. Tamarisk Treatment in the Mojave River Watershed. Ken Lair. , Lair Restoration Consulting. Hesperia, CA. Chuck Bell and Jackie Lindgren. , . Mojave Desert Resource Conservation District. Victorville, CA. La gamme de thé MORPHEE vise toute générations recherchant le sommeil paisible tant désiré et non procuré par tout types de médicaments. Essentiellement composé de feuille de morphine, ce thé vous assurera d’un rétablissement digne d’un voyage sur . 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 .