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Outflowing Molecular Gas in NGC 3079
Published online by Cambridge University Press: 12 April 2016
Abstract
NMA 12CO(J=1-0) observations of the radio lobe spiral galaxy, NGC 3079, reveal a dense, rigidly rotating ring of molecular gas with a radius of about 750 pc. In addition, a tilted CO component as well as several molecular gas “spurs” are interpreted as linear features which are accelerated outwards by the nuclear outflow.
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- 3. Astronomical Results and Prospects
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- Copyright © Astronomical Society of the Pacific 1994