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High-Frequency Study of Low and Intermediate Luminosity Radio Galaxies

Published online by Cambridge University Press:  25 May 2016

L. Gregorini
Affiliation:
1 Istituto di Radioastronomia del CNR - Bologna, Italy
P. Parma
Affiliation:
1 Istituto di Radioastronomia del CNR - Bologna, Italy
U. Klein
Affiliation:
3 Radioastronomisches Institut der Universität Bonn - Germany
K.-H. Mack
Affiliation:
3 Radioastronomisches Institut der Universität Bonn - Germany

Extract

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All the information on the morphology, spectral index and polarization properties of low and intermediate luminosity radio galaxies were collected in an intermediate frequency range, and some of the basic questions to be elucidated with such measurements are still unanswered. We therefore decided to extend the study of their characteristics towards higher frequencies. From the B2 and 4C catalogue we selected 26 radio galaxies for which VLA or WSRT data are available. These sources were observed at 10.6 GHz using the Effelsberg 100-m telescope (Gregorini & al. 1992; Mack & al. 1994; Klein & al. 1995).

Type
Properties of Radio Sources
Copyright
Copyright © Kluwer 1996 

References

Gregorini, L., Klein, U., Parma, P., Schlickeiser, R., Wielebinski, R. (1992) High-frequency radio continuum observations of low-luminosity radio galaxies I. A sample of sources with angular sizes > 4′, Astron. Astrophys. Suppl. Ser. , Vol. no. 94, pp.1335 Google Scholar
Jägers, W.J. (1986), The polarization of radio galaxies, , Google Scholar
Mack, K-H., Gregorini, L., Parma, P. Klein, U. (1994) High-frequency radio continuum observations of radio galaxies with low and intermediate luminosity II. Sources with sizes 4′ to 5′, Astron. Astrophys. Suppl. Ser. , Vol. no. 103, pp. 157182 Google Scholar
Klein, U., Mack, K-H., Gregorini, L., Parma, P. (1995) High-frequency radio continuum observations of radio galaxies with low and intermediate luminosity III. Spectral indices and particle ages Astron. Astrophys., in press Google Scholar