Hostname: page-component-848d4c4894-v5vhk Total loading time: 0 Render date: 2024-06-16T14:48:29.144Z Has data issue: false hasContentIssue false
  • English
  • Français

A bisymmetric spiral magnetic field in the Milky Way

Published online by Cambridge University Press:  04 August 2017

Y. Sofue  and
M. Fujimoto
Y. Sofue
Affiliation:
Nobeyama Radio Observatory, Tokyo Astronomical Observatory, and A. von Humboldt Fellow at the MPI für Radioastronomie Bonn
M. Fujimoto
Affiliation:
Department of Physics, Nagoya University

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.

The distribution of Faraday rotation measure (RM) of extragalactic radio sources shows that a large-scale magnetic field in the Galaxy is oriented along the spiral arms. The field lines change direction from one arm to the next in the inter-arm region.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 251 - 252
Copyright
Copyright © Reidel 1985 

References

Sofue, Y., and Fujimoto, M.: 1983, Astrophys. J. 265, 722 CrossRefGoogle Scholar
Tabara, H., and Inoue, M.: 1981, Publ. Astron. Soc. Japan 33, 603 Google Scholar