Detection of spiral magnetic fields in two flocculent galaxies

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dc.creatorKnapik, J.
dc.creatorSoida, M.
dc.creatorDettmar, R. -J.
dc.creatorBeck, R.
dc.creatorUrbanik, M.
dc.date2000-09-27
dc.date.accessioned2026-07-07T01:55:39Z
dc.date.available2026-07-07T01:55:39Z
dc.descriptionTwo flocculent galaxies NGC 3521 and NGC 5055 has been observed at 10.55GHz with the Effelsberg 100m telescope. In both cases polarized emission reveals substantial radial component of regular magnetic field - similar to that in grand-designed spirals. Comparison with H_alpha distribution obtained at Lowell Observatory is presented. Polarization models discussed, support modern non-standard dynamo concepts for magnetic field generation in galaxies.
dc.description11 pages, 10 figures, A&A in print
dc.identifierhttps://arxiv.org/abs/astro-ph/0009438
dc.identifierhttp://arxiv.org/abs/astro-ph/0009438
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1733
dc.subjectAstrophysics
dc.titleDetection of spiral magnetic fields in two flocculent galaxies
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