Large, highly organized radio structures near the galactic centre

Details Large, highly organized radio structures near the galactic centre Large, highly organized radio structures near the galactic centre

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.310..557y&link_type=abstract

Nature (ISSN 0028-0836), vol. 310, Aug. 16, 1984, p. 557-561.

Astronomy and Astrophysics

Astronomy

270

Astronomical Maps, Galactic Nuclei, Galactic Radio Waves, Milky Way Galaxy, Radio Sources (Astronomy), Centimeter Waves, Filaments, Interstellar Gas, Interstellar Magnetic Fields, Morphology, Very Large Array (Vla)

Scientific paper

A radio map of the galactic centre made at a wavelength of 20 cm with the Very Large Array telescope reveals that most of the radio emission arising within 50 pc of the galactic centre is not associated with ionizing radiation from recently formed stars. Rather, the large-scale geometry and the measured polarization of the radio emission strongly suggest that the nonthermally emitting gas is arranged along magnetic structure indicative of a substantial poloidal component to the magnetic field in the central region of the Galaxy.

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