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Astronomy and Astrophysics

Volumn 494, Issue 1, 2009, Pages 1-9

Studying the leptonic structure of galaxy cluster atmospheres from the spectral properties of the SZ effect

(3) Colafrancesco, S a,b,c Prokhorov, D d,e Dogiel, V f

a ESA ESRIN (Italy)

b ASI (Italy)

c INAF OSSERVATORIO ASTRONOMICO DI ROMA (Italy)

d MOSCOW INSTITUTE OF PHYSICS AND TECHNOLOGY (Russian Federation)

e INSTITUT D'ASTROPHYSIQUE DE PARIS (France)

f LEBEDEV PHYSICAL INSTITUTE (Russian Federation)

Author keywords

Cosmology: cosmic microwave background; Cosmology: theory; Galaxies: clusters: general

Indexed keywords

COSMOLOGY; ELECTRONS; GALAXIES; HOLOGRAMS; KINEMATICS; MICROWAVES; PROGRAMMING THEORY; THERMIONIC EMISSION; VANADIUM COMPOUNDS;

A THERMALS; COSMIC STRUCTURES; COSMOLOGY: COSMIC MICROWAVE BACKGROUND; COSMOLOGY: THEORY; CROSS-OVER FREQUENCIES; ELECTRON DISTRIBUTIONS; ELECTRON POPULATIONS; FREQUENCY RANGES; GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; NON THERMALS; OPTIMAL FREQUENCIES; PECULIAR VELOCITIES; POWER LAWS; SPECTRAL PROPERTIES; SPECTRAL SLOPES; STOCHASTIC ACCELERATIONS; SYSTEMATIC BIAS; SZ EFFECTS;

ATMOSPHERIC SPECTRA;

EID: 59449099398 PISSN: 00046361 EISSN: 14320746 Source Type: Journal
DOI: 10.1051/0004-6361:200810111 Document Type: Article

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