Comptonization of the cosmic microwave background by high energy particles residing in AGN cocoons

Astronomy and Astrophysics

Volumn 520, Issue 15, 2010, Pages

  Prokhorov, D A ^a   Antonuccio Delogu, V ^b,c   Silk, J ^d,e  

^a Korea Astronomy and Space Science Institute (KASI)   (South Korea)

^b INAF OSSERVATORIO ASTROFISICO DI CATANIA   (Italy)

^c SCUOLA SUPERIORE DI CATANIA   (Italy)

^d UNIVERSITY OF OXFORD   (United Kingdom)

^e INSTITUT D'ASTROPHYSIQUE DE PARIS   (France)

Author keywords

cosmic background radiation; galaxies: cluster: intracluster medium; galaxies: ISM; radiative transfer; relativistic processes

Indexed keywords

COMPUTER SIMULATION; COSMOLOGY; DIELECTRIC MATERIALS; GALAXIES; HIGH ENERGY PHYSICS; INTERFEROMETERS; MATHEMATICAL MODELS; MONOLITHIC MICROWAVE INTEGRATED CIRCUITS; NUMERICAL METHODS; POPULATION STATISTICS; RADIATIVE TRANSFER; RADIO ASTRONOMY; SPECTROSCOPY; X RAYS;

2-D NUMERICAL SIMULATION; 2D SIMULATIONS; ACTIVE GALACTIC NUCLEI; ANALYTIC MODELS; CHANDRA; COMPTONIZATION; COSMIC BACKGROUND RADIATION; COSMIC MICROWAVE BACKGROUNDS; ENERGETIC ELECTRON; GALAXIES: CLUSTERS; GALAXIES: ISM; GAS TEMPERATURE; HIGH FREQUENCY; HIGH TEMPERATURE; HIGH-ENERGY ELECTRON; HIGH-ENERGY PARTICLES; INTENSITY MAPS; INTENSITY SPECTRUM; JOINT ANALYSIS; LOW ENERGIES; NONTHERMAL; NUMERICAL SIMULATION; PRESSURE VALUES; RADIO INTERFEROMETERS; RADIO MAPS; RADIO SOURCES; RELATIVISTIC CORRECTION; RELATIVISTIC ELECTRON; RELATIVISTIC PROCESSES; SELF-SIMILAR; SPECTRAL FUNCTION; SZ EFFECTS; X-RAY CAVITIES; X-RAY MISSION;

PRESSURE EFFECTS;

EID: 77957970637     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913920     Document Type: Article

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