PPT-Quasar 95

Club dastronomie de Frouville Mesures de focales JeanPierre Maratrey octobre 2014 Au menu Différentes méthodes de mesure de focale des lentilles minces Mesure à linfini Relation de conjugaison. edu Abstract Cloud computing promises 64258exibility and high performance for users and high costef64257ciency for operators Neverthe less most cloud facilities operate at very low utilization hurting both cost effectiveness and future scalability We . . . . 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. Redshifts. Gordon Richards. Drexel University. With thanks to. Michael Strauss, . Xiaohui. Fan, Don Schneider, and . Linhua. Jiang. Quasar Luminosity Function. Croom. et al. 2004. Space density of quasars as a function of . With thanks to the members of the Quasar Working Group, particularly Don Schneider, . Xiaohui. Fan, Michael Strauss, Pat Hall, Dan . Vanden. . Berk. , Sebastian Jester, and . Scott Anderson, also Adam Myers. February 9, 2013. @ 11:00 am. T. he unusually bright centers found in some galaxies are called . a. ctive galactic nuclei.. s. tarbursts.. h. alos.. s. upermassive. black holes.. According to current understanding, what is a quasar?. M87. Hercules A radio jets. Active Galactic Nuclei (AGNs) and Supermassive Black Holes. The identification by Maarten Schmidt (1963, . Nature. , 197, 1040) of the radio source 3C 273 as a . “. star. Reionization. . Chris . Carilli (NRAO). LANL Cosmology School, July . 2011. . Review: constraints on IGM during . reionization. CMB large scale polarization. Gunn-Peterson effect. Quasar near zones: . Roberto Maiolino. Feedback is the key:. - reducing SF efficiency . . (gas . heating+turbulence. ). - removing baryons. Discrepancy . between halo . mass . functions . and stellar/baryons mass function. Acceleration of Quasar-Driven Galactic Winds. and on the . Density Structure of the CGM. Jonathan Stern (MPIA. ). Alexander von Humboldt Fellow. May 2016. Papers. :. 1. Stern, . Laor. & Baskin (2014a), MNRAS... A Single Form, Mixing Diagram,. and Outliers . Heng Hao (SISSA). Martin Elvis (CFA). and COSMOS Team. INAF-OABO . Seminar. 2012-10-25 . 10%. 90%. Outline. Introduction: Definition . and Important Questions . Division of Particle and Astrophysical Science, Nagoya University, JAPAN. with. SKA-Japan high-. z. galaxy and cosmology WG. East-Asian SKA WS, 30 . Nov. .-2 Dec., 2011, KASI, . Daejeon. , Korea. Formation and Evolution of Galaxies:. Mark Kidger. European Space Agency. European Space Astronomy Centre. Herschel Science Centre. What is a Quasar?. Quasar is a contraction of . Quasi-Stellar Object. .. They are objects that look like faint, blue stars, but are really incredibly distant.. Here’s the Story We’ll Unfold for You…. Hubble’s galaxy classifications: Spirals, . ellipticals. , irregulars. . Structural parts of galaxies: disk, halo, nucleus, bulge. Spiral arms – tracers of star formation. Charles L. Steinhardt. 1. , . Heng. . Hao. 2. , . Monica . Young. 3. , . Guido Risaliti. 4. , . Francesca . Civano. . Harvard-Smithsonian . Center. for Astrophysics. and. 1. IPMU, Univ. Tokyo; 2..