Radio halos in future surveys in the radio continuum

Astronomy and Astrophysics

Volumn 548, Issue , 2012, Pages

  Cassano, R ^a   Brunetti, G ^a   Norris, R P ^c   Rottgering H J A ^d   Johnston Hollitt, M ^b   Trasatti, M ^e  

^a INAF ISTITUTO DI RADIOASTRONOMIA   (Italy)

^b VICTORIA UNIVERSITY OF WELLINGTON   (New Zealand)

^c CSIRO   (Australia)

^d LEIDEN UNIVERSITY   (Netherlands)

^e UNIVERSITY OF BONN   (Germany)

Author keywords

Galaxies: clusters: general; Radiation mechanisms: non thermal; Radio continuum: general; X rays: general

Indexed keywords

GALAXIES: CLUSTERS: GENERAL; GALAXY CLUSTERS; LOW AND HIGH FREQUENCIES; LOWER FREQUENCIES; LUMINOSITY FUNCTIONS; MASSIVE SYSTEMS; MONTE CARLO SIMULATION; NONTHERMAL; PHENOMENOLOGICAL APPROACH; RADIATION MECHANISMS: NONTHERMAL; RADIO CONTINUUM; RADIO CONTINUUM: GENERAL; RADIO FREQUENCIES; RADIO HALO; RE-ACCELERATION; RED SHIFT; STATISTICAL PROPERTIES; STEEP SPECTRA; SYNCHROTRON SOURCE; THEORETICAL MODELS; THEORETICAL PREDICTION; X-RAYS: GENERAL;

GALAXIES; LUMINANCE; MERGING; MONTE CARLO METHODS;

SURVEYS;

EID: 84870367240     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220018     Document Type: Review

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