| dc.contributor.author | Bailey, J. | |
| dc.contributor.author | Axon, D.J. | |
| dc.contributor.author | Hough, J. | |
| dc.contributor.author | Ward, M.J. | |
| dc.contributor.author | McLean, I. | |
| dc.contributor.author | Heathcote, S.R. | |
| dc.date.accessioned | 2009-04-17T14:03:20Z | |
| dc.date.available | 2009-04-17T14:03:20Z | |
| dc.date.issued | 1988 | |
| dc.identifier.citation | Bailey , J , Axon , D J , Hough , J , Ward , M J , McLean , I & Heathcote , S R 1988 , ' The polarization of NGC 1068 ' , Monthly Notices of the Royal Astronomical Society , vol. 234 , no. 4 . | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | dspace: 2299/3201 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3201 | |
| dc.description | Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA] | |
| dc.description.abstract | Broad-band polarimetry of NGC 1068 over the wavelength range 0.36 - 4.8 μm is presented, together with high-resolution spectropolarimetry of the Hβ, [O III] and Hα, [N II] regions of the spectrum. The authors recognize several different polarization components and conclude that they can all be accounted for by processes involving dust. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | The polarization of NGC 1068 | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
