Volume 330, Issue 2-3 pp. 133-136
Original Paper

Polarimetric observations of a sample of Compact Steep-Spectrum sources

F. MantovaniK.-H. Mack

K.-H. Mack

Istituto di Radioastronomia – INAF, Via Gobetti 101, 1-40129, Bologna, Italy

Search for more papers by this author
F. M. Montenegro-Montes

F. M. Montenegro-Montes

Istituto di Radioastronomia – INAF, Via Gobetti 101, 1-40129, Bologna, Italy

Dpto. de Astrofísica. Universidad de La Laguna, Avda. Astrofísico Fco. Sánchez s/n, E-38200 La Laguna, Spain

Instituto de Astrofísica de Canarias. C/ Via Láctea s/n. E-38200 Tenerife, Spain

Search for more papers by this author
A. Rossetti

A. Rossetti

Istituto di Radioastronomia – INAF, Via Gobetti 101, 1-40129, Bologna, Italy

Search for more papers by this author
A. Kraus

A. Kraus

Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

Search for more papers by this author
First published: 13 February 2009

Abstract

Measurements of the polarised emission from Compact Steep-Spectrum (CSS) sources can give important information about the physical conditions inside and around the region of radio emission, essentially on the Narrow Line Region. We have observed the sample of CSS sources constructed by Fanti et al. (1990) with the Effelsberg 100-m radio telescope at four frequencies between 2.7 GHz and 10.4 GHz in order to measure the polarisation parameters. Results from the NRAO VLA Sky Survey (Condon et al. 1998) at 1.4 GHz were combined with our measurements for the full sample. The sample is considered statistically complete and allows comprehensive statistical analysis. Some of our conclusions are in disagreement with previous results obtained by polarimetric observations of other samples, for example the B3-VLA sample (© 2009 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

The full text of this article hosted at iucr.org is unavailable due to technical difficulties.