Strong asymmetries in the radio galaxy 3C 337 and its large-scale emission-line gas

Details Strong asymmetries in the radio galaxy 3C 337 and its large-scale emission-line gas Strong asymmetries in the radio galaxy 3C 337 and its large-scale emission-line gas

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98.1232p&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 98, Oct. 1989, p. 1232-1245.

Astronomy and Astrophysics

Astronomy

33

Astronomical Spectroscopy, Emission Spectra, Galactic Structure, Interstellar Gas, Radio Galaxies, Astronomical Maps, Asymmetry, Gray Scale, Line Spectra

Scientific paper

Detailed multifrequency VLA observations of the high-luminosity radio galaxy 3C 337 reveal a source that is highly asymmetric in its structural, luminosity, spectral, and polarization properties. Extensive emission-line regions are seen to the east of the galaxy, where the radio source shows signs of interaction with an external medium, such as strong depolarization and a double hotspot. These results are discussed in the context of a clumpy two-phase thermal medium around distant radio galaxies and its importance for their structure.

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