Hostname: page-component-586b7cd67f-l7hp2 Total loading time: 0 Render date: 2024-11-26T21:29:51.284Z Has data issue: false hasContentIssue false
  • English
  • Français

Multifrequency Polarimetry of CSS Sources

Published online by Cambridge University Press:  19 July 2016

Everton Lüdke ,
Chidi E. Akujor  and
Simon T. Garrington
Everton Lüdke
Affiliation:
NRAL-Jodrell Bank, Cheshire, SK11 9DL, UK
Chidi E. Akujor
Affiliation:
NRAL-Jodrell Bank, Cheshire, SK11 9DL, UK
Simon T. Garrington
Affiliation:
NRAL-Jodrell Bank, Cheshire, SK11 9DL, UK

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Compact Steep Spectrum Sources (CSS) have projected linear sizes < 20 kpc and overall steep spectrum (5 ∼ v −α, α ≥ 0.6). Interactions with a dense interstellar medium may confine the CSSs and produce the high amounts of Faraday rotation that some distorted sources present. The first results of a detailed study of the multifrequency polarization properties of a sample of CSS sources with MERLIN and the VLA are presented.

Type
Poster Contributions: Polarisation
Information
Symposium - International Astronomical Union , Volume 159: Multi-Wavelength Continuum Emission of AGN , 1994 , pp. 471
Copyright
Copyright © Kluwer 1994 

References

[1] Kato, T., Tabara, H., Ionue, M. and Aizu, K. 1987, Nature , 329, 223 Google Scholar
[2] van Breugel, W.J.M. et al 1992, A&A 256, 56 Google Scholar