Hostname: page-component-745bb68f8f-v2bm5 Total loading time: 0 Render date: 2025-01-29T17:25:34.510Z Has data issue: false hasContentIssue false
  • English
  • Français

The Magnetic Field of M 51

Published online by Cambridge University Press:  19 July 2016

N. Neininger ,
C. Horellou ,
R. Beck ,
E.M. Berkhuijsen ,
M. Krause  and
U. Klein
N. Neininger
Affiliation:
Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn 1, FRG
C. Horellou
Affiliation:
DEMIRM, Observatoire de Meudon, France
R. Beck
Affiliation:
Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn 1, FRG
E.M. Berkhuijsen
Affiliation:
Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn 1, FRG
M. Krause
Affiliation:
Max–Planck–Institut für Radioastronomie, Auf dem Hügel 69, W-5300 Bonn 1, FRG
U. Klein
Affiliation:
Radioastronomisches Institut der Universität, Auf dem Hügel 71, W-5300 Bonn 1, FRG

Extract

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.

We present observations of the polarized emission and the derived magnetic field structure of the spiral galaxy M 51 at different wavelengths: 2.8 cm, 6.2 cm, 18 and 20.5 cm.

Type
7. Magnetic Fields in Galaxies: Observations
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 313 - 314
Copyright
Copyright © Kluwer 1993 

References

Horellou, C., Beck, R., Berkhuijsen, E.M., Krause, M., Klein, U.: 1992, A & A 265, 417 Google Scholar
Neininger, N.: 1992, A & A 263, 30 Google Scholar