PPT-AGN dust model of 3CR sources

MIR imaging amp s pectroscopy ISM dust model amp PAH vectorized Monte Carlo model SED of a clumpy AGN torus Frank Heymann PhD Martin Haas Endrik Kr. 2 Fugitive Dust Sources Significant atmospheric dust arises from the mechanical disturbance of granular material exposed to the air Dust generated from these open sources is termed fugitive because . 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. 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. Dr. Kyle Perry, P.E.. PEM Seminar – September 5, 2014. Dry Dust. Respirable Dust Problems. Wet Dust . Caking Problems. Proprietary Dust. 2 Types. Newly Developed Dust. Hydrophobic. Research Funded by Kentucky Department for Energy Development and Independence (DEDI). 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. 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 . 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. . OR. WHY IN THE WORLD DID THEY STAY?. Mapping the Dust Bowl. RELIEF AND LOAN SERVICES: KERC, JULY 25, 1934. Agricultural Adjustment Act. Regional Production Corporation. Farm Credit Administration. Emergency Crop and Feed Loans. RWS1301. Lang/Phil/Culture. PHIL 3206. Creative Arts. MUSL 1327. HIST 1301. HIST 1302. POLS 2310. POLS 2311. SCI 1301. COMM 1301. Soc & . Beh. Sci. PSYC 1301. MATH 1411. MATH 1312 or. STAT 2480. The. . XMM ultra-deep survey in the CDFS. . Andrea Comastri . INAF-Osservatorio Astronomico Bologna ITALY. P. Ranalli (UniBO), R. Gilli (INAF-BO), C. Vignali (UniBO),. K. Iwasawa (ICC-Barcelona), I. Georgantopoulos (INAF-BO), N. Cappelluti (INAF-BO), E. Rovilos (INAF-BO), X. Barcons (IFCA), F.J. Carrera (IFCA), S. Falocco (IFCA), M. Brusa (MPE), H. Brunner (MPE), I. Balestra (MPE), A. Merloni (MPE), A. Finoguenov (MPE), F. Civano (CfA), F. Fiore (INAF-Roma), F. Nicastro (INAF-Roma), S. Puccetti (ASI), V. Mainieri (ESO), P. Rosati (ESO), P. Tozzi (INAF-TS), N. Brandt (PSU), J. Silverman (IPMU). 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 .