Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-24T21:03:01.445Z Has data issue: false hasContentIssue false
  • English
  • Français

The Full “Alpha-Tensor” Due to Supernovae and Superbubbles in the Galactic Disk

Published online by Cambridge University Press:  19 July 2016

K. M. Ferrière
K. M. Ferrière*
Affiliation:
High Altitude Observatory National Center for Atmospheric Research P.O. Box 3000 Boulder, CO 80307-3000

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.

We provide a simple and realistic expression for the alpha-tensor in the Galactic disk, when turbulence is driven by supernova explosions and superbubbles.

Type
9. Magnetohydrodynamic Phenomena in the Interstellar Medium Related to Dynamo Processes
Information
Symposium - International Astronomical Union , Volume 157: The Cosmic Dynamo , 1993 , pp. 383 - 387
Copyright
Copyright © Kluwer 1993 

References

Ferrière, K. M. 1993, ApJ, 404, (submitted) Google Scholar
Heiles, C. 1987, ApJ, 315, 555 CrossRefGoogle Scholar
Kennicutt, R. C. Jr., Edgar, B. K., & Hodge, P. W. 1989, ApJ, 337, 761 CrossRefGoogle Scholar
Moffatt, H. K. 1978, in “Magnetic Field Generation in Electrically Conducting Fluids” (Cambridge: Cambridge Univ. Press)Google Scholar
Parker, E. N. 1971, ApJ, 163, 255 CrossRefGoogle Scholar
Stone, R. C. 1981, AJ, 86, 544 CrossRefGoogle Scholar