Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-20T03:48:46.853Z Has data issue: false hasContentIssue false

Origin of Magnetic Fields in Jets and Radio Galaxies

Published online by Cambridge University Press:  19 July 2016

William K. Rose*
Affiliation:
Astronomy Program University of Maryland College Park, MD 20854, U.S.A.

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.

Jets are known to be emitted from the centers of active galaxies and quasars. In two recent papers (Rose, 1987, 1989) calculations of magnetic fields generated in jets because electrons drift with respect to protons have been described. Electron drift velocities can result from interaction with the cosmic background radiation or with ambient gas. We describe how magnetic fields can be generated in jets and radio galaxies.

Type
8. The Role of Magnetic Fields in Radio Source Jets and Extended Radio Lobes
Copyright
Copyright © Kluwer 1990 

References

Rose, W.K. (1987) Astrophys. J. 313, 146 (Paper I).Google Scholar
Rose, W.K. (1989) Astrophys. J. 337, 91 (Paper II).CrossRefGoogle Scholar
Rose, W.K., Beall, J.H., Guillory, J. and Kainer, S. (1987) Astrophys. J. 314, 95.CrossRefGoogle Scholar
Rose, W.K., Guillory, J., Beall, J.H. and Kainer, S. (1984) Astrophys. J. 280, 550.Google Scholar