Modeling the Generation of the Magnetic Field in NGC 5775

Details Modeling the Generation of the Magnetic Field in NGC 5775 Modeling the Generation of the Magnetic Field in NGC 5775

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002arep...46..871s&link_type=abstract

Astronomy Reports, Vol. 46, Issue 12, pp. 871-873

Astronomy and Astrophysics

Astronomy

4

Scientific paper

A model for the generation of large-scale magnetic fields is constructed for the galaxy NGC 5775, in which the magnetic field has the form of a dipolar dynamo wave propagating along the galactic disk. The excitation of such a mode, which is unusual for galactic dynamos, can be explained by the strong variation of the galactic rotation with height above the plane of symmetry of the galactic disk.

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