PPT-Les Pulsars gamma avec GLAST
Author : pasty-toler | Published Date : 2016-06-26
David Smith Centre dEtudes Nucléaires de BordeauxGradignan CENBG in2p3 CNRS I nstitut de Physique Nucléaire de Lyon 6 mars 2015 Le ciel en rayons gamma avec
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Les Pulsars gamma avec GLAST: Transcript
David Smith Centre dEtudes Nucléaires de BordeauxGradignan CENBG in2p3 CNRS I nstitut de Physique Nucléaire de Lyon 6 mars 2015 Le ciel en rayons gamma avec le satellite Fermi . Introduction to pulsars Pulsars are rotating neutron stars born Pulsars are rotating neutron stars born from core collapse of Type II from core collapse of Type II supernova supernova Periods of p Dan Hooper . - . Fermilab. /University of Chicago University of Michigan Dark Matter Workshop, April . 1. 5. . th. , 2013. Dark Matter in The Galactic Center. The volume surrounding the Galactic Center is complex; backgrounds present are not necessarily well understood . TERRA PRETA. Objectif:. . Guérir la terre pour être en bonne santé. Pratique:. . Comment faire de la Terra preta pour son balcon, son jardin et pour le sol agricole. L’homme est . encore en . . 22/10/2011 INDIGO . discussions@IUCAA. . Bhal. Chandra Joshi . Radio pulsar searches . Radio pulsars - highly magnetized rotating NS - compact . - periodic pulses . R. N. Manchester. CSIRO Astronomy and Space Science Australia . Telescope National Facility. , Sydney. Summary. Pulse profiles – doubles and . interpulses. High . Edot. pulsars – radio and high-energy emission. The Pulsar Search Collaboratory. Questions We Will Answer. What is a . pulsar. ?. Why do astronomers study pulsars?. What is the . PSC. ?. How can . you. get involved?. What is a pulsar?. A pulsar is a . Sergei Popov. (SAI MSU). Plan. General intro. Pulsar models. Population synthesis. Summary of discoveries. EGRET legacy. Just 6 pulsars:. Crab. Geminga. Vela. PSR B1055-52. PSR B1706-44 . PSR B1951+32 . Enrico Bozzo. University. of Geneva. Transitional pulsars pulsations at unprecedentedly low X-ray Luminosities. XSS 12270-4859. P. spin. = 1.69 ms. L. X. = 5x10. 33. erg/s. (. Papitto. et al. 2015) . CE1. Déroulement . : . ❶ . Expression . orale autour du . th. è. me, oral collectif . :. * . Lecture . offerte. . d’albums en . lien avec le thème abordé dans le dessin de . Ludo au coin regroupement.. T. AVEC. i. AVEC. E. Tautogramme. Tautogramme. Tautogramme. Tautogramme. Tautogramme. Tautogramme. Beau. Un(e. ) nom commun . qui joue de la/le . nom commun. Questions / réponses. Savez-vous ce qui est. 4.1.7 DAQ & FSWV5Gunther HallerSLACLAT Chief Electronics EngineerDAQ & Flight Software Systems Managerhaller@slac.stanford.edu(650) 926-4257 ray Large ray Large Area Space Area Space TelescopeTelescop V21Flight Software WBS 417Gunther Hallerhallerslacstanfordedu650 926-4257ray Large ray Large Area Space Area Space TelescopeTelescopeGLAST LAT Project417V22Stand Summary Stand Summary Finished TKR/CAL North Bengal University. TeV Neutrinos and Gamma rays from Pulsars/Magnetars. Introduction. The energy spectrum of cosmic rays extends to extremely high energies, values exceeding 10. 20. . eV. .. The origin of the cosmic rays and the mechanism responsible for acceleration of cosmic rays to such high energies . Jocelyn Bell . Burnell. University of Oxford Astrophysics . And. Mansfield College. 1957. 2. 3. Crab PSR almost discovered I. Late . summer 1957; . an Open Night . at McDonald; . 82 inch . (Struve) telescope .
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