Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-25T18:16:19.467Z Has data issue: false hasContentIssue false

Magnetic fields in irregular galaxies

Published online by Cambridge University Press:  01 November 2008

Amanda Kepley
Affiliation:
Department of Astronomy, University of Wisconsin–Madison, 475 N. Charter St., Madison, WI 53704, USA email: [email protected], [email protected], [email protected], [email protected]
Eric Wilcots
Affiliation:
Department of Astronomy, University of Wisconsin–Madison, 475 N. Charter St., Madison, WI 53704, USA email: [email protected], [email protected], [email protected], [email protected]
Ellen Zweibel
Affiliation:
Department of Astronomy, University of Wisconsin–Madison, 475 N. Charter St., Madison, WI 53704, USA email: [email protected], [email protected], [email protected], [email protected]
Stefanie Mühle
Affiliation:
Stichting JIVE, Postbus 2, 7990 AA Dwingeloo, The Netherlands email: [email protected]
John Everett
Affiliation:
Department of Astronomy, University of Wisconsin–Madison, 475 N. Charter St., Madison, WI 53704, USA email: [email protected], [email protected], [email protected], [email protected]
Timothy Robishaw
Affiliation:
School of Physics, The University of Sydney, NSW 2006, Australia email: [email protected]
Carl Heiles
Affiliation:
Astronomy Department, University of California, Berkeley, California 94720-3411, USA email: [email protected]
Uli Klein
Affiliation:
Argelander-Institut für Astronomie, Universität Bonn, Auf dem Hügel 71, D-53121 Bonn, Germany email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The low masses of irregular galaxies change the behavior of their interstellar medium (ISM) compared to that of normal spirals, so the role of magnetic fields in the ISM in irregulars may be very different than in spirals. We present high-resolution and high-sensitivity observations of the magnetic fields of two irregular galaxies: NGC 4214 and NGC 1569.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Allsopp, N. J. 1979, MNRAS 188, 765CrossRefGoogle Scholar
Chyży, K. T., Beck, R., Kohle, S., Klein, U., & Urbanik, M. 2000, A&A 355, 128Google Scholar
Chyży, K. T., Knapik, J., Bomans, D. J., Klein, U., Beck, R., Soida, M., & Urbanik, M. 2003, A&A 405, 513Google Scholar
Ferrière, K. & Schmitt, D. 2000, A&A 358, 125Google Scholar
Gaensler, B. M., Haverkorn, M., Staveley-Smith, L., Dickey, J. M., McClure-Griffiths, N. M., Dickel, J. R., & Wolleben, M. 2005, Science 307, 1610CrossRefGoogle Scholar
Klein, U., Haynes, R. F., Wielebinski, R., & Meinert, D. 1993, A&A 271, 402Google Scholar
Mao, S. A., Gaensler, B. M., Stanimirovic, S., Haverkorn, M., McClure-Griffiths, N. M., Staveley-Smith, L., & Dickey, J. M. 2008, arXiv:0807.1532Google Scholar
Martin, C. L. 1998, ApJ 506, 222CrossRefGoogle Scholar
Westmoquette, M. S., Smith, L. J., & Gallagher, J. S. 2008, MNRAS 383, 864CrossRefGoogle Scholar