Hostname: page-component-77c89778f8-9q27g Total loading time: 0 Render date: 2024-07-23T11:23:17.292Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Fields in the Irregular Galaxy LMC

Published online by Cambridge University Press:  19 July 2016

Richard Wielebinski
Richard Wielebinski*
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn 1, FRG

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.

New radio continuum surveys allowed the determination of the magnetic field in the Large Magellanic Cloud. The magnetic field is filamentary, extending to the south of the 30 Doradus nebula. Some possible explanations for this unusual morphology are discussed.

Type
7. Magnetic Fields in Galaxies: Observations
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 317 - 319
Copyright
Copyright © Kluwer 1993 

References

Haynes, R.F. et al.: 1991, A&A 252, 475 Google Scholar
Klein, U. and Gräve, R.: 1987, in Beck, R., Gräve, R., ed(s)., Interstellar Magnetic Fields , Springer: Berlin, p. 76 CrossRefGoogle Scholar
Klein, U., Weiland, H. and Brinks, E.: 1991, A&A 246, 323 Google Scholar
Klein, U., Haynes, R.F., Wielebinski, R., Meinert, D.: 1992, A&A (submitted) Google Scholar
Luks, T. and Rohlfs, K.: 1992, A&A 263, 41 Google Scholar
Mathewson, D.S. and Ford, V.L.: 1970, ApJ 75, 778 CrossRefGoogle Scholar
Murai, T. and Fujimoto, M.: 1980, PASJ 32, 581 Google Scholar
Schmidt, Th.: 1970, A&A 6, 294 Google Scholar
Schmidt, Th.: 1976, A&AS 24, 357 Google Scholar
Wayte, S.R.: 1990, ApJ 355, 473 CrossRefGoogle Scholar