The coma cluster magnetic field from faraday rotation measures

Astronomy and Astrophysics

Volumn 513, Issue 5, 2010, Pages

  Bonafede, A ^a,b   Feretti, L ^b   Murgia, M ^b,c   Govoni, F ^c   Giovannini, G ^a,b   Dallacasa, D ^a,b   Dolag, K ^d   Taylor, G B ^e,f  

^a UNIVERSITY OF BOLOGNA   (Italy)

^b INAF ISTITUTO DI RADIOASTRONOMIA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI CAGLIARI   (Italy)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^e UNIVERSITY OF NEW MEXICO   (United States)

^f NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

Author keywords

Galaxies: clusters: general; Galaxies: clusters: individual: A1656 Coma; Magnetic fields; Polarization

Indexed keywords

GALAXIES; MAGNETIC FIELDS; POLARIZATION; POWER SPECTRUM; RADIO ASTRONOMY; ROTATION; THREE DIMENSIONAL;

CENTRAL MAGNETIC FIELD; CONFIDENCE LEVELS; FARADAY ROTATIONS; FIELD SCALE; GALAXIES: CLUSTERS: GENERAL; GALAXIES: CLUSTERS: INDIVIDUAL: A1656 COMA; GAS DENSITY; KOLMOGOROV; MAGNETIC FIELD STRENGTHS; NUMERICAL SIMULATION; POLARIZATION DATA; POWER-LAW; RADIAL PROFILES; RADIO SOURCES; SCALE RESOLUTION; THREE DIMENSIONAL MAGNETIC FIELDS; VERY LARGE ARRAYS;

MAGNETIC MATERIALS;

EID: 77951129778     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913696     Document Type: Article

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