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Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect

The measurement of Zeeman splitting in spectral lines---both in emission and absorption---can provide direct estimates of the magnetic field strength and direction in atomic and molecular clouds, both in our own Milky Way and in external galaxies. This method will probe the magnetic field in the warm and cold neutral components of the interstellar medium, providing a complement to the extensive SKA Faraday studies planning to probe the field in the ionized components.

preprint2015arXivOpen access
Timothy RobishawJames A. GreenGabriele SurcisWouter VlemmingsA. M. S. RichardsSandra EtokaTyler BourkeVincent FishMalcolm GrayHiroshi ImaiBusaba KramerJames McBrideEmmanuel MomjianAnuj SarmaAlbert Zijlstra
astro-ph.GA
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Open access15 authors1 topic
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Timothy RobishawJames A. GreenGabriele SurcisWouter VlemmingsA. M. S. RichardsSandra EtokaTyler BourkeVincent FishMalcolm GrayHiroshi ImaiBusaba KramerJames McBrideEmmanuel MomjianAnuj SarmaAlbert Zijlstra

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