The polarization of radio galaxies: Its structure at low frequencies

Details The polarization of radio galaxies: Its structure at low frequencies The polarization of radio galaxies: Its structure at low frequencies

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phdt.........5j&link_type=abstract

Ph.D. Thesis Leiden Univ. (Netherlands).

Astronomy and Astrophysics

Astronomy

28

Low Frequencies, Radio Astronomy, Radio Galaxies, Astronomical Models, Elliptical Galaxies, Galactic Clusters, Galactic Radio Waves, Galactic Structure, Quasars

Scientific paper

The 0.6 GHz mapping of extended radio galaxies: edge-brightened double sources; edge-darkened double sources; 3C66B, NGC1265, 3C129, DA240, 3C236, 4C48.29, IC708 and IC711, 4CT51.29.1, 3C310, Abell2256, 3C402 and 3C465; systematics of spectral index distributions of radio sources at low frequencies, and systematics of polarization distributions (evidence for excess gas associated with giant elliptical galaxies) is summarized. A multifrequency polarization study of 3C66B is described. Low frequency polarization observations of the radio galaxy 4C73.48; radio observations of the giant quasar 4C34.47; the cluster around 3C130; the radio structure of 3C130 interpreted with a dynamical model; and possible one-sized ejection in the prototype tailed radio galaxy 3C129 are considered.

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