High frequency radio observations of the Stephan's Quintet region

Details High frequency radio observations of the Stephan's Quintet region High frequency radio observations of the Stephan's Quintet region

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.253..176k&link_type=abstract

Nature, vol. 253, Jan. 17, 1975, p. 176, 177.

Astronomy and Astrophysics

Astronomy

8

Microwave Interferometers, Point Sources, Radio Sources (Astronomy), Astronomical Maps, Astronomical Models, Astronomical Spectroscopy, Extragalactic Radio Sources, Galactic Nuclei, Radio Astronomy, Radio Galaxies

Scientific paper

In the case of Stephan's Quintet, observations at 1.415 GHz suggest an arc-shaped source partially encircling a point source centered on NGC7319. A three-element interferometer was used at frequencies of 2.695 and 8.085 GHz to synthesize areas centered at a point near Stephan's Quintet. Results of 2.695 GHz observations superimposed on a 200-inch print of Stephan's Quintet are presented. The latest observations do not reveal the arc structure.

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