The large radio galaxy DA 240: Evidence for jets?

Details The large radio galaxy DA 240: Evidence for jets? The large radio galaxy DA 240: Evidence for jets?

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981esasp.162...83s&link_type=abstract

In ESA Opt. Jets in Galaxies p 86-86 (SEE N81-27993 18-88)

Mathematics

Logic

3

Galactic Structure, Jets, Plasma Jets, Radio Galaxies, Astronomical Photography, Collimation, Gas Flow, Line Spectra, Radio Emission

Scientific paper

Optical and radio observations of DA 240 are presented which suggest that there is a collimated structure in its outer components. A probable morphological connection is noted between the outer radio emission and the optical jet in the central galaxy MCG 9-13-57. This system and NGC 5128/Cen A have striking features in common including a strong indication that the gas flowing in the jet contains thermal material and is moving nonrelativistically. The fact that optical jets are narrow, often embedded in diffuse emission and include a blue continuum gives the Space Telescope clear advantages over ground based instruments.

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