Detecting the largest magnets - The universe and the clusters of galaxies

Astronomy and Astrophysics – Astronomy

Scientific paper

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Galactic Clusters, Galactic Evolution, Intergalactic Media, Interstellar Magnetic Fields, Dynamo Theory, Galactic Rotation, Magnetic Flux, Quasars, Sky Surveys (Astronomy), Spiral Galaxies

Scientific paper

Recently, a large sample of rotation measures of galaxies and quasars at various redshifts has been published. This data set is used to test for the existence of an uniform component of a cosmic/intergalactic magnetic field outside clusters of galaxies. From a total of 309 galaxies and quasars with a known redshift and a small intrinsic rotation measure value, an upper limit of about 2 rad/sq m is obtained for such a cosmic/intergalactic contribution out to a redshift z of 3.6. From this result, and a mean density of 0.00001/cu cm, an upper limit of 6 x 10 to the -12th G follows for the strength of such a cosmic/intergalactic magnetic field outside clusters of galaxies, or an upper limit of 6 x 10 to the -11th G for a mean density of 10 to the -6th/cu cm.

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