Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...351l...9e&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 351, March 1, 1990, p. L9-L12.
Astronomy and Astrophysics
Astronomy
58
Galactic Evolution, Infrared Astronomy, Radio Galaxies, Red Shift, Astronomical Photometry, Infrared Imagery, Radio Sources (Astronomy)
Scientific paper
J (1.2-micron) and K (2.2 micron) images have been obtained for eight 3CR radio galaxies with redshifts from 0.7 to 1.8. Most of the objects were known to have extended asymmetric optical continuum or line emission aligned with the radio lobe axis. In general, the IR morphologies of these galaxies are just as peculiar as their optical morphologies. For all the galaxies, when asymmetric structure is present in the optical, structure with the same orientation is seen in the IR and must be accounted for in any model to explain the alignment of optical and radio emission.
Chokshi Arati
Eisenhardt Peter
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