Abstract
New radio continuun observations are used to investigate the connection between magnetic fields and the spiral structure in the nearby grand design galaxy M51. Compression of magnetic field in shock fronts is probably the origin of the strong regular magnetic field in the spiral arms. The origin of the almost equally strong inter-arm regular magnetic field is less clear.
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Beck, R., Brandenburg, A., Moss, D., Shukurov, A., & Sokoloff, D. 1996, ARA&A 34, 155
Gómez, G.C. & Cox, D.P. 2002, ApJ 580, 235
Martos, M.A. & Cox, D.P. 1998, ApJ 509,703
Regan, M.W., Thornley, M.D., Helfer, T.T., et al. 2001, ApJ 561, 218
Rots, A.H., Bosma, A., van der Hulst, J.M., et al. 1990, AJ 100, 387
Tubbs, A.D. 1980, ApJ 239, 882
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© 2004 Kluwer Academic Publishers
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Fletcher, A., Beck, R., Berkhuijsen, E.M., Horellou, C., Shukurov, A. (2004). Magnetic Fields and Spiral Structure. In: Alfaro, E.J., Pérez, E., Franco, J. (eds) How does the Galaxy Work?. Astrophysics and Space Science Library, vol 315. Springer, Dordrecht. https://doi.org/10.1007/1-4020-2620-X_60
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DOI: https://doi.org/10.1007/1-4020-2620-X_60
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-2619-5
Online ISBN: 978-1-4020-2620-1
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