Polarization in CSS/GPS radio sources
| dc.creator | Dallacasa, D. | |
| dc.date | 2004-12-13 | |
| dc.date.accessioned | 2026-07-07T02:16:15Z | |
| dc.date.available | 2026-07-07T02:16:15Z | |
| dc.description | The polarisation properties of the intrinsically small (< 20 kpc) radio sources are briefly discussed. At centimetric and decimetric wavelengths, substantial polarised emission is often detected in quasars and, at a lower level, in radio sources identified with galaxies with projected linear sizes in excess of a few kpc. The projected linear size at which some polarised emission is detected decreases with observing frequency. High Rotation Measures are commonly found in these sources, implying high electron/ion densities and/or strong interstellar magnetic fields. For the objects found unpolarized at resolutions of the order of a few pc, either the source magnetic field is highly disordered or the scale of ambient magnetic field cells is not resolved. | |
| dc.description | 6 pages. 2 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 59-64. Needs evn2004.cls | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0412299 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0412299 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8716 | |
| dc.subject | Astrophysics | |
| dc.title | Polarization in CSS/GPS radio sources | |
| dc.type | text |