Cosmic magnetic fields in galaxies, groups and clusters

Details Cosmic magnetic fields in galaxies, groups and clusters Cosmic magnetic fields in galaxies, groups and clusters

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..259..569g&link_type=abstract

Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium,

Mathematics

Logic

Galaxies: Clusters: General, Galaxies: Magnetic Fields, Magnetic Fields, Radio Continuum: Galaxies, Polarization, Methods: Data Analysis

Scientific paper

The distribution of the Faraday depth induced by galaxies, groups and clusters on a patch of sky is investigated. For instance, we utilise a halo model approach to obtain synthetic Faraday skies. Moreover, our modelling includes cluster physical as well as cosmological aspects. A SKA sky survey will provide a large sample of rotation measures of polarised sources. Hence, we examine to what extent statistics of rotation measures of these sources can yield information about cosmic magnetic fields and cosmology.

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