Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aj.....88..709h&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 88, June 1983, p. 709-758.
Astronomy and Astrophysics
Astronomy
132
Astronomical Maps, Galactic Clusters, Intergalactic Media, Quasars, Radio Sources (Astronomy), Astronomical Models, Galactic Evolution, Red Shift, Tables (Data)
Scientific paper
The possibility that quasars may occur as members of clusters or groups of galaxies has important implications for the interpretation of the quasar phenomenon and for studies of galaxy and cluster evolution. Available data support the hypothesis that the distorted radio morphologies of both 1400+162 and 3C275.1 are due to interaction with dense intracluster media. In connection with these results, the present investigation is concerned with a VLA snapshot survey of 3C, 4C, and Molonglo QSOs in order to identify objects showing distortions in their radio maps. To ensure a high percentage of resolved sources, observations were primarily conducted of objects in several low-frequency surveys, taking into account the 3C, 3CR, 4C, and two Molonglo surveys. Observations of over 120 quasars were obtained during VLA runs on November 23, 1980, and April 23, 1981. It was found that a significant portion of radio QSOs are distorted or 'bent' triple sources. On the other hand, the distortions observed may not all be due to interactions with external media.
Hintzen Paul
Owen Frazer
Ulvestad Jim
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