Origin of the galactic centre lobes

Details Origin of the galactic centre lobes Origin of the galactic centre lobes

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985natur.317..699u&link_type=abstract

Nature (ISSN 0028-0836), vol. 317, Oct. 24, 1985, p. 699-701.

Physics

53

Galactic Evolution, Galactic Nuclei, Galactic Structure, Radio Galaxies, Accretion Disks, Lobes, Stellar Evolution

Scientific paper

Recent observations of the 10-GHz continuum have indicated that there is a pair of lobes having ridges of intensity extending from the galactic centre region in a direction perpendicular to the galactic plane. The authors interpret these lobes as being due to a magnetodynamic acceleration mechanism in which the production and relaxation of the magnetic twist induced by the rotation of the contracting gas disk play a part. The plasma is accelerated in a conical cylinder with a helical velocity field, reproducing the observed feature of radio lobes.

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