Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-29T18:30:01.919Z Has data issue: false hasContentIssue false

Large Scale Magnetohydrodynamical Considerations in Spiral Galaxies

Published online by Cambridge University Press:  04 August 2017

E. Battaner
Affiliation:
Instituto de Astrofísica de Andalucía. CSIC. Apdo. 2144. Granada
M. L. Sánchez-Saavedra
Affiliation:
Dpto. Física Fundamental. Universidad de Granada. (Spain)

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.

A magnetohydrodynamical result is deduced, which could contribute to our understanding of spiral and ring structures in galaxies. The usual expressions for the continuity, momentum and induction equations are adopted for the gas of a galaxy, and the following simplifying hypotesis are made : a) Steady state conditions, b) Axisymmetry, c) A velocity field given by (π=0, θ=θ(r), Z=0) for the interstellar gas (where π,θ and Z are the radial, azimuthal and vertical to the galactic plane components and r is the distance from the galactic center). Then, the direction of magnetic field must be azimuthal and the plasma distribution is compatible with ring structures.

Type
II. Spiral Structure
Copyright
Copyright © Reidel 1983 

References

Battaner, E. and Sánchez-Saavedra, M.L.: 1982, Astron. and Space Sci. 86, 55.Google Scholar