The role of radial motions and WARPS of the disk in the Galactic dynamo

Details The role of radial motions and WARPS of the disk in the Galactic dynamo The role of radial motions and WARPS of the disk in the Galactic dynamo

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991mvsfa..32...71z&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 3 - Fizika, Astronomiia (ISSN 0579-9392), vol. 32, Mar.-Apr. 1991, p. 71-76. In Russian.

Astronomy and Astrophysics

Astronomy

Milky Way Galaxy, Perturbation Theory, Radial Velocity, Rotating Disks, Spiral Galaxies, Astronomical Models, Dynamo Theory, Interstellar Gas, Interstellar Magnetic Fields

Scientific paper

Perturbation theory is used to examine the influence of warps of the disk and radial streams on the dynamo in a thin disk. With reference to the Galaxy as well as to the spiral galaxies M51 and M81, it is found that the role of these two factors is small. The weak influence of the radial streams is explained by the character of their radial dependence, while the role of the disk warps is basically reduced to an effective change in the rotation curve.

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