The Magnetic Field of the Large Magellanic Cloud: A New Way of Studying Galactic Magnetism

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dc.creatorGaensler, Bryan M.
dc.creatorHaverkorn, M.
dc.creatorStaveley-Smith, L.
dc.creatorDickey, J. M.
dc.creatorMcClure-Griffiths, N. M.
dc.creatorDickel, J. R.
dc.creatorWolleben, M.
dc.date2005-03-16
dc.date.accessioned2026-07-07T02:17:14Z
dc.date.available2026-07-07T02:17:14Z
dc.descriptionWe present a study of the Faraday rotation of extragalactic sources lying behind the Large Magellanic Cloud. These data represent the most detailed study yet of magnetic field structures in any external galaxy, and are a demonstration of how magnetic fields in galaxies will best be studied with future instruments.
dc.description9 pages, 5 embedded EPS figures, uses krakproc.cls . To appear in conference proceedings "The Magnetized Plasma in Galaxy Evolution", eds. K. T. Chyzy et al
dc.identifierhttps://arxiv.org/abs/astro-ph/0503371
dc.identifierhttp://arxiv.org/abs/astro-ph/0503371
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9102
dc.subjectAstrophysics
dc.titleThe Magnetic Field of the Large Magellanic Cloud: A New Way of Studying Galactic Magnetism
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