Cross-like radio structure in NGC 6500 - Evidence for bipolar outflow?

Details Cross-like radio structure in NGC 6500 - Evidence for bipolar outflow? Cross-like radio structure in NGC 6500 - Evidence for bipolar outflow?

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...208...14u&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 208, no. 1-2, Jan. 1989, p. 14-16.

Astronomy and Astrophysics

Astronomy

13

Active Galaxies, Radio Jets (Astronomy), Radio Sources (Astronomy), Astronomical Maps, Emission Spectra, Spiral Galaxies, Very Large Array (Vla)

Scientific paper

NGC 6500 is one of a small group of mildly active galaxies which show radio structure elongated both along and perpendicular to the galactic disk. New high-resolution MERLIN and VLA maps of this complex radio source are presented. The maps are consistent with a model in which radio emission is generated by the outflow of material along the galactic minor axis. This outflow is not comparable to the highly-collimated radio jets seen in some active galaxies, but is probably similar to the wind-driven bipolar outflow seen in M 82.

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